Transcript
RRS James Clark Ross Cruise JR106
Autosub under Arctic Sea Ice
Cruise Report Peter Wadhams, Steve Ackley, Ken Collins, Pat Cooper, Terry Edwards, Jeffrey Evans, Gwyn Griffiths, Nick Hughes, Arthur Kaletzky, Steve McPhail, Duncan Mercer, Colm Ó Cofaigh, Kieran Rutherford, Andy Webb, Jeremy Wilkinson, Guy Williams and Doug Willis
Grant NER/T/S/2000/00985
Autosub under Arctic Sea Ice
JR106 Cruise Report (v1.00)
CONTENTS CONTENTS ...............................................................................................................................2 INTRODUCTION .....................................................................................................................3 SCIENTIFIC STAFF .................................................................................................................4 PURPOSE OF CRUISE.............................................................................................................6 CRUISE NARRATIVE .............................................................................................................7 AUTOSUB MISSION SUMMARY LOG ..............................................................................18 AUTOSUB NAVIGATION SYSTEM PERFORMANCE .....................................................19 AUTOSUB COLLISION AVOIDANCE................................................................................20 AUTOSUB HOMING SYSTEM AND ACOUSTIC TRACKING ........................................22 AUTOSUB MECHANICAL REPORT...................................................................................24 AUTOSUB SCIENTIFIC SENSORS......................................................................................28 AUTOSUB - KONGSBERG EM2000 MULTIBEAM SWATH SYSTEM ...........................31 AUTOSUB POST-PROCESSED NAVIGATION DATA FORMAT ....................................35 AUTOSUB ADCP DATA DEFINITION (JR106) .................................................................36 SEA ICE VALIDATION PROGRAMME..............................................................................39 SATELLITE DATA ................................................................................................................40 SEA ICE WATCH...................................................................................................................45 PHYSICAL OCEANOGRAPHY............................................................................................49 MARINE TECHNOLOGY TESTS .........................................................................................58 ALONG TRACK MEASUREMENTS ...................................................................................60 EM120 MULTIBEAM SWATH BATHYMETRY AND TOPAS .........................................62 SHIPBOARD ADCP ...............................................................................................................71 LADCP.....................................................................................................................................74 CONTINUOUS PLANKTON RECORDER...........................................................................76 ITS REPORT ...........................................................................................................................77 APPENDIX A - ICE STATION DATA..................................................................................79 APPENDIX B – SALINITIES .................................................................................................89 APPENDIX C – LADCP SCRIPTS AND PROCESSING MESSAGES ...............................90
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INTRODUCTION Peter Wadhams (DAMTP/SAMS) Cruise JR106a was the second of four planned cruises by James Clark Ross to be carried out for the NERC Autosub-under-Ice (AUI) programme. The first cruise was in 2003 towards Pine Island Bay in the Antarctic. The third, in fact the second leg of JR106 (JR106b), is to south-east Greenland in September 2004; the fourth, JR97, will be to the Weddell Sea in January 2005. The purpose of AUI is to obtain data from beneath sea ice, glacier tongues and ice shelves using Autosub, and to develop Autosub’s capabilities as a cryospheric research tool. During the cruise reported here the Autosub was operated highly successfully under both moving pack ice and fast ice, obtaining some 400 km of high quality upward looking swath sonar data as well as oceanographic data. It undertook necessary avoidance manoeuvres for both deep pressure ridges and shallow seabed hazards in a classical manner as designed, and procedures for use of the acoustic homing system were developed to the point where the vehicle could be returned with confidence to an area covered with loose moving pack ice in the knowledge that it could be sent to a holding pattern out of which it could be steered towards the ship and recovered. This is a cause of increased confidence for the future use of the vehicle in regions covered with sea ice. Thanks are due to Steve McPhail and the entire AUV technical team for the quiet efficiency and hard work which underlay every mission and which was the chief cause of success. We are grateful for the contribution of all the other scientific groups on board, including the ice drilling teams, the ice watch, the SPRI group which ran the swath sonar system, and the CTD operators. We thank those who came as observers – Steve Ackley, Ken Collins and Gwyn Griffiths – but who willingly undertook onerous watchkeeping tasks. Especial thanks are due to the Captain, Chris Elliott, and the officers and crew of James Clark Ross for their unending support. We are grateful also to the Alfred Wegener Institute and to Professor Peter Lemke for the assistance of Polarstern in the ice thickness validation exercise on 25 August. For help in Reykjavik we offer special thanks to Professor Ingibjorg Jonsdottir, University of Iceland. The cruise was carried out under NERC grant NER/T/S/2000/00985 to Professor Peter Wadhams at Department of Applied Mathematics and Theoretical Physics, University of Cambridge, currently on leave at Dunstaffnage Marine Laboratory, Oban.
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SCIENTIFIC STAFF Peter Wadhams
DAMTP/SAMS
[email protected]
Jeremy Wilkinson Nick Hughes Duncan Mercer Russell Ladkin Arthur Kaletzky Gwyn Griffiths James Perrett Kieran Rutherford Mark Squires Andrew Webb Dave White Peter Stevenson Stephen McPhail Dr. Colm O Cofaigh Dr. Jeffrey Evans Ruth Mugford Ken Collins Zoe Roberts Terry Edwards Guy Williams Steve Ackley Pat Cooper Doug Willis
SAMS SAMS SAMS SAMS DAMTP Autosub Autosub Autosub Autosub Autosub Autosub Autosub Autosub SPRI SPRI SPRI SOC SOC UKORS ACECRC USA BAS BAS
[email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected] [email protected]
SAMS –
Scottish Association for Marine Science Dunstaffnage Marine Laboratory Oban Argyll PA37 1QA Scotland
DAMTP –
University of Cambridge, Department of Applied Mathematics and Theoretical Physics Centre for Mathematical Sciences Wilberforce Road Cambridge CB3 0WA United Kingdom
Autosub –
Autosub Mission Team Southampton Oceanography Centre Waterfront Campus European Way Southampton SO14 3ZH United Kingdom
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SPRI –
Scott Polar Research Institute University of Cambridge Lensfield Road Cambridge CB2 1ER United Kingdom
SOC –
Southampton Oceanography Centre Waterfront Campus European Way Southampton SO14 3ZH United Kingdom
UKORS –
United Kingdom Ocean Research Services Southampton Oceanography Centre Waterfront Campus European Way Southampton SO14 3ZH United Kingdom
ACECRC -
Antarctic Climate and Ecosystems Co-operative Research Centre Marine Ecosystems Group University of Tasmania Private Bag 80 Hobart 7001 Australia
USA -
Clarkson University Potsdam, New York.
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PURPOSE OF CRUISE Peter Wadhams The purpose of the cruise was to obtain ice thickness distributions from the upwardlooking swath sonar system aboard Autosub, to validate the thickness values against other data collected simultaneously from the surface and the air, and to conduct transects across and within Fram Strait so as to obtain estimates of ice flux. An important aspect of the cruise also was the developme nt of operating methods which are suitable for ice-covered waters. The moving sea ice in Fram Strait in August 2004, following a long period of calm weather, was a very diffuse cover which spread far to the east but with a coverage of only 12/10. This was an unfavourable type of ice for Autosub for three reasons. Firstly the low concentration meant that not much ice was profiled per hard-won mile of Autosub mission track, with additional problems arising from the extensive calm water causing a loss of lock in the sonar (described later by Arthur Kaletzky). Secondly, the concentration, while diffuse, was sufficient to make surfacing of the Autosub dangerous, so the homing system had to be (and was) developed much further than before to allow the vehicle to return to a point, circle submerged, then be led out to the ship which places herself in the nearest available open water. Thirdly, the overall distances involved were so great that even a series of Autosub missions would not suffice to cross the very large width of the East Greenland Current in Fram Strait that was affected by ice. For these reasons, after initial experiments, the decision was made to move to the fast ice edge for more intensive experiments and validation work. This has many positive advantages. The fast ice edge was well defined by satellite imagery, and the fast ice comprised formerly moving ice which had become pinned to certain shoals, and so comprised all kinds of ice (first and multi year, undeformed and ridged) at 100% concentration. The fact that it was stationary meant that the planned helicopter coverage of the Autosub tracks by the helicopter-borne EM system of Polarstern need not take place at the exact time, or even on the same day, as the Autosub mission. Unfortunately, on the day of Polarstern’s visit, fog conditions did not allow more than minimal flying. Nevertheless, the surface EM and drilling validations could be fitted more exactly to the Autosub tracks, given that the sea ice platform was not moving. Supporting work included along-track ice monitoring using the manual watch system developed for the ASPeCt programme in the Antarctic; some CTDs over the NE Greenland shelf, particularly in the Belgica Trough just south of Nordostrundingen which forms a part of the Northeast Water Polynya in winter; continuous operation of the Simrad swath sounding sonar system from the ship; tests of the SAMS Homer; and deployment of a Nagurny ice thickness buoy and a Hardy continuous plankton recorder.
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CRUISE NARRATIVE Peter Wadha ms AUGUST 10, TUESDAY The group based at SAMS (Peter Wadhams, Jeremy Wilkinson, Nick Hughes) and at DAMTP (Arthur Kaletzky) arrived in Reykjavik from Glasgow and London respectively, and moved into apartments of the University of Iceland kindly provided through Prof. Ingibjorg Jonsdottir, formerly Peter’s student. The weather in Reykjavik was sunny and intensely hot, more than 30°C, a long-term record. AUGUST 11, WEDNESDAY James Clark Ross arrived in the morning from her previous cruise for Woods Hole Oceanographic Institution around south Greenland, and moored in inner harbour. The day was spent dealing with the agents, Nesskip, and locating our equipment. More scientists arrived. James Clark Ross offloaded the Woods Hole scientists and equipment. AUGUST 12, THURSDAY James Clark Ross began loading equipment for the new cruise in the morning, and scientists were able to move aboard in the afternoon. The ship was visited by Professor Detlef Quadfasel, Institut für Meereskunde, University of Hamburg, whose group was joining A.V. Humboldt for a cruise to Denmark Strait together with a group from SAMS. AUV technical team were hard at work preparing Autosub for operation, and carried out a float test over the stern in the harbour, to test ballasting of vehicle. The weather continued hot and sunny. AUGUST 13, FRIDAY Most people spent the morning enjoying the final hours of an extraordinary week of Mediterranean weather in Iceland. A huge number of outdoor cafes enjoyed a vast and unexpected clientele. By coinc idence the only cloud seen for four days began to appear as we prepared for departure, and soon low cloud filled the sky to provide a more normal Icelandic environment. James Clark Ross sailed at 1600 (all times in GMT), passing out of the harbour between the French cruise ship Le Diamant and the Danish ocean patrol vessel Vaedderen which herself was bound for NE Greenland. Outside the harbour the pilot boat Jotunn departed with the pilot, leaving us to cope with an offshore fog bank through which large numbers of fishing vessels loomed. While James Clark Ross handled this tricky navigational problem there was a safety briefing for the scientists, featuring lifejackets, immersion suits, alarm signals, getting into lifeboats, and watertight doors. At 1830 we streamed the Hardy-Longhurst continuous plankton recorder, to obtain a continuous transect up to and from Fram Strait. This was a project for Dr. Chris Reid of the Alister Hardy Research Foundation, Plymouth. Position was 64°23.72’N, 22°40.30’W. Swath bathymetric mapping began, manned by the SPRI group, and continued throughout the voyage.
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In the evening we saw the volcano of Snaefellsnes to starboard, covered with snow, in a sunny twilight. AUGUST 14, SATURDAY A scientific meeting was held at 1000 to organise the cruise and assign watches. I arranged general watches as 6-on-6-off with Jeremy Wilkinson, Nick Hughes and Guy Williams on 0000-0600, 1200-1800; and myself, Duncan Mercer and Russell Ladkin on 0600-1200, 1800-2400. The general watch-keepers do CTDs, ice work, general coordination and processing. Steve Ackley is looking after the ice observations log, using the ASPeCt system (developed for the Antarctic) with Kieran Rutherford (Gwyn’s student), Ken Collins, Guy Williams and Gwyn Griffiths. Zoe Roberts is assisting the three SPRI personnel doing multibeam watch-keeping. The AUV team set up their own system of working together independent of fixed hours. Along-track logging of all environmental parameters was under way; Nick reprogrammed the logging system on the ship’s ADCP. One XBT is taken per day in support of the swath bathymetry, which is now showing iceberg scours on the Icelandic shelf. Late in the evening the sun’s image distorted itself into a mirage as it sank into a perfectly calm Greenland Sea at 2220. I thought I saw the green flash, but as usual my eyes probably deceived me. As the sun sank, some low lying very distant land was silhouetted. A look at the chart showed that this was part of Knud Rasmussen Land in Greenland, just south of Kap Brewster, and that it was some 25 miles away. Noon position 67°08.3’N, 23°35.6’W. AUGUST 15, SUNDAY Contact was established by email with Peter Lemke, Chief Scientist of Polarstern, and plans evolved for our joint work later in the cruise. In the evening I gave a talk on the background to the cruise in relation to climate change in the Arctic. The ship progressed to the NE. Sea calm, but not as flat calm as yesterday. Fiery sunset again at 10.30 pm. Cassette in plankton recorder changed today at 1045 am; a single cassette lasts for 500 nautical mile (n.ml.). Noon position 70°48.9’N, 15°08.9’W. AUGUST 16, MONDAY Finally established direct radio contact with Polarstern, at 83°N in the Arctic Ocean, and set up a daily radio schedule at 1000 with Lemke. Held scientific meeting at 1000 to plan tomorrow’s work when first experiments start. We are receiving three types of satellite imagery daily (QuikSCAT and two types of AMSR) via an Iridium link with Danish Technical University (Dr. Leif Toudal) with further wide-swath Envisat from Richard Hall, Norsk Polarinstitutt. Copies of all images are passed to the bridge. Thanks to this wealth of sea ice information it was possible to see that we would have to modify our initial goal of running a transect at 78°50’N from E to W, crossing the moored upward sonar systems of Norsk Polarinstitutt for validation, and continuing W. NERC Grant NER/T/S/2000/00985
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This year the ice in Fram Strait is extremely diffuse, and the imagery showed no significant ice east of 6°W at 78° 50’N. We made this our initial goal and decided to work westward from there towards a wide band of fast ice which still existed against the Greenland coast. At 1940 the first ice was seen – a thin tabular berg originating from the Flade Isblink. Position was 76°37.0’N, 7°14.0’W. It showed up well on radar. A further berg was visible on radar ahead at 76°54.1’N, 7°13.6’W. We began to see very diffuse ice all around – eroded brash and blocks of old ice. The ice watch was started. At 2150 the plankton recorder was brought in because of possible ice hazard. It was very calm with little or no wind and a lazy swell. Many internal wave slicks were visible – evidence of a thin surface melt layer from melting ice which has not mixed down because of absence of wind. Surface salinity was a very low 29.63. Noon position 75°03.5’N, 8°13.6’W. AUGUST 17, TUESDAY We spent the night threading our way slowly through an ice promontory which extended unusually far E at a lower latitude than Fram Strait. This slowed us to the point where we could not expect to reach 78°50’N today. In order to give the AUV a full day of initial tests we stopped at 77°37’N, 3°07’W and started work there. Three missions were carried out during the day (358, 359 and 360). In the first, the AUV went into the water and did preliminary test of systems, then a test of acoustic tracking and homing systems. Problems with telemetry meant that the AUV surfaced after 40 minutes at the start way point. Then we ran the ship 6 n.ml. westward into the ice and deployed Autosub to run eastward out to the original site (which was in nearly open water with just occasional small cakes and brash). This was mission 359. We followed with the ship, running a video system and keeping an intensive ice log along the track. This gave us the first partially validated under- ice data, although the ice concentration was only about 10-20%. Finally the AUV did more tests at the outer site (mission 360), on the homing system. The vehicle ho med at 1 km and 12 km range. We looked at the sonar data from mission 359 and found that although floes were clearly visible and resolvable in shape and thickness, the topography was superimposed on a parabolic false contour which ranged from zero at the mid- line to 20 m at extreme slant range. We set out to examine the theoretical reasons for this, and it was tentatively assigned to a loss of lock caused by the mirror- like sea surface, the low reflectivity of open water, and the very open nature of the icefield. Noon position 76°36.6’N, 3°06.2’W. AUGUST 18, WEDNESDAY We headed N overnight (although there is no darkness) in open water for rapid transit to get to 78°50’N by breakfast time. In fact this meant that the ship sailed far to the E to avoid all ice, which greatly added to our journe y time. Most of the day was spent trying to recoup our position. We sailed to 78°50’N at 1°W then headed directly W, in fog and very diffuse ice, at no greater than 6 kts. The news from Polarstern is that AWI has instructed her
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to head back N to 83° and recover and clean up the remains of the abandoned Russian ice station NP32 which they passed earlier. This will delay our rendezvous. During the afternoon we crossed the longitudes of the NPI moorings (at 4-6°W), but the AUV could not be launched as the ice, although diffuse, was sufficiently uniform in floe spacing that there was no hole large enough for a safe retrieval at this early stage in homing system development. The same applied to three tabular icebergs which were embedded in the pack ice. Finally we reached the continental shelf, passing the last NPI mooring position at 6°W. At a water depth of 305 m we were able to do an AUV run to NW, towards fast ice edge observed on satellite imagery. This is because at these water depths the vehicle can use bottom tracking rather than dead reckoning, which greatly increase the precision of retrieval, While the AUV was in the water we did the first CTD (1045) at 78°50.7’N, 6°25.0’W. This showed polar surface layer with the Atlantic layer (200 m peak at 2.0°C) below it penetrating onto the shelf. Some surface warming had occurred, so polar water temperature minimum of –1.8°C was at 100 m. The AUV run, again under diffuse drift ice, yielded 6 n.ml.of data (mission 361). We then continued NW towards the fa st ice edge through frustrating ice, too dense for safe AUV operation but not dense enough to really provide a good test for AUV. Noon position 78°48.0’N, 0°43.20’W. AUGUST 19, THURSDAY At 0050 we manoeuvred to bring the AUV in from mission 361, then we set off NW towards a sharp ice edge, probably fast ice edge, shown by satellite imagery. At 0107 our position was 78°50.6’N, 6°26.1’W. I ran the digital video recorder from the bridge as we ran along the track followed yesterday by the AUV. Jeremy took over watch while I got a small amount of sleep until 0600. At 0630 we stopped in an opening of more than average open water to do CTD (water depth 170 m) and see if this is a good launch site for AUV. Ice cover was still only 2-3/10, but with larger floes (50 m or so), mostly first-year with melt pools. The CTD was complete by 0715 and Steve McPhail engaged in preparing for an Autosub mission. Several problems occurred with the software, so at 1430 we set off towards the ice edge while they were still being resolved. At 1708 we came across a very wide large multiyear floe some 1 mile across, which looked like broken-out fast ice. We decided to do an AUV test, but could see many tabular icebergs behind it, so sailed round it so as to launch AUV outwards from behind the floe and avoid danger of hitting iceberg. Also the floe drift was eastward and would have brought the floe over the launch site. We did a CTD in 189 m of water just before this manoeuvre then launched AUV. While it was in the water we closely inspected a tilted tabular iceberg, near us, with pockmarked surface, veined dirt- filled cracks down side, and faintly green appearance. It was at 79°27.6’N, 9°31.1’W. The AUV mission (362) was 3 n.ml. out, 3 n.ml. back, crossing the big floe. We launched at 2010. Upon recovery we headed for this mass of big tabular bergs with a view to surveying with AUV. Found that this is actually a shoal on which they are stranded. One that we came close to had a freeboard of 11-11.5 m, thus a possible draft of up to 80 m, and
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was in 93 m of water. It didn’t seem to move. There were no fewer than 12 icebergs together in a great mass, most tabular, but with one white randomly shaped berg obviously from the Arctic Basin. We sailed through them, finding 83–100 m of water and thus are pretty sure that they are aground. But still this is a good site for getting SAR imagery for an iceberg detection study. We carried on to NW after extensive photography. Noon position 79° 15.6’N, 8° 22.9’W. AUGUST 20, FRIDAY I rose at 6 after only 3 hours sleep to find us still running NW towards fast ice edge as shown by satellite imagery. The ice cover was very open indeed, almost pure open water, although tabular icebergs littered the scene – six in sight. At 0619 we reached 79°29.8’N, 13°12.4’W. At 0400 am we had done an along-track CTD in about 200 m of water. At 0700 I recorded iceberg positions on radar and found 9 that I could correlate with visual observation. By 0708 we were at 79°30.1’N, 13°55.5’W and were now heading due W towards the ice edge, which soon appeared as a white line in the distance, with further tabular icebergs clearly embedded within it and the mountains of NE Greenland looming faintly in the far background. At 0718 I ordered a CTD, although the water depth was only about 100 m. By about 0830 we reached the fast ice edge, behind which lay a continuous sheet of what looked like thick first-year or thin multi- year ice, with occasional ridges and many melt pools. I called Steve and proposed a long Autosub mission into the fast ice. He planned a 20 hour mission – 30 miles in and back. The chart shows 35 miles from the ice edge westward to the beginning of shoaling water on the W side of the Belgica Trough, so all seemed OK. He got down to the task of preparation. At 1000 I called Peter Lemke. Polarstern had successfully salvaged the abandoned Russian NP32 camp, saving 300 drums of fuel, but this had put them back. They cannot reach us until August 25, but the advantage of them doing the surveys then is that they can do them all in one go – because we are dealing with fast ice there is no longer the necessity of doing simultaneous helicopter and AUV profiles. His present position was 80°36’N, 2°21’W. Finally, after lunch, Autosub was launched (mission 363), submerged quickly and set off. We moved the ship into the fast ice edge at what we calculated was the exact point of entry of Autosub and started an ice characterisation exercise. First workers on the ice were Jeremy, Duncan, Nick and me. We went over the side in a weird rope buoy contraption labelled “Wor Geordie”. We laid out a line of holes at 5 m intervals for 100 m, and drilled away until the drill got stuck. At this very moment a fog bank came in and we were recalled to the ship since polar bears would be invisible (a watch was being kept from the bridge). We had to leave the drill, 2 m of flights and the power head on the ice. After dinner the fog had cleared, so we went out again with Steve Ackley and Ken. The drill released itself easily, and we went on to complete 40 holes (2 x 100 m rows at 5 m intervals) and take a core. Typical ice thicknesses were 1.6-1.8 m. Towards the end we were advised that Autosub had reappeared, so we finished off quickly and set out to locate it. It was found and interrogated. It had encountered a 60 m water depth somewhere and had been programmed to turn round and come out if this happened, so it was doing the correct thing.
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Noon position 79°30.0’N,14°24.2’W. AUGUST 21, SATURDAY The decision was to send Autosub into ice again at midnight for a 12 hour run on the same track as on the 20th but shallower depth (30 m) and with more depth tolerance. During night we would do swath bathymetry locally. At 0800 we would get back to ice edge for ice work. The reality was quite similar. The AUV did get into water soon after midnight (mission 364). Then we did swath bathymetry. At 0800 we started listening for AUV (not due until after 1200) and it turned up. It had been turned back quite early by a 25 m pressure ridge, with little data acquired, and had been hanging around the way point for hours. We recovered the AUV at 0910 in some minor grease ice which had formed during night, and the AUV team started changing the battery pack, a 6 hour task. They found that the previous mission, on Aug 20, had been turned back at 79°28.02’N, 15°20.54’W. It had generated a 136 m swath width, which looked good, but which needs validation. At 1000 I called Peter Lemke and found that Polarstern was at 78°50’N, 01°50’W, picking up moorings. They said bad weather was forecast (up to force 7 to 8) overnight and on Sunday, according to their onboard meteorologist. Peter is sending email of weather forecast to us. Then we went out to do ice work. We forced way into ice a little forward of previous position. We extended yesterday’s ice line from 100 m to a further 100 m (away from ice edge) and added a 100 m cross 50 m along new section. We did two cores. We stayed out over lunch with hot dogs and chips lowered to us. 6 people did it: usual gang (me, Duncan, Jeremy, Nick) plus Ken Collins and Zoe. We came back aboard. and talked to Steve about the next mission. Then we tried drilling again, to do cores in a dirty ice area in front of ship (multi- year?). Visibility was marginal, but we did 2 cores in area of dirty ice, photographed the layout of melt pools, laid out new cross line at end of 200 m main line, did snow depths but then were called in because the AUV was ready to go. The AUV went into the water at 1840. It did a float test first because of change of batteries. Then it dived and went off. We started a bathy swath again. Noon position 79°29.9’N, 14°24.8’W. AUGUST 22, SUNDAY The situation as of 0730 was that during the night, when we listened for the AUV at 0100 and 0700 (due back 1840) and did bathymetric swaths between times, the wind, far from breaking up the fast ice, packed in the moving ice against it. This created a band of close pack against the fast ice edge. This allowed the ship to be forced off the listening site until we were now a mile away. The wind was still strong, and the prospect was for more pack ice to move in and for the ship to move further away until it is out of listening range of the recovery position (79°30’N, 14°20.5’W).
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We did a CTD, suffering a delay while the tracking winch was fixed. We finished CTD at 1140 then listened – no signal yet. We went N for 90 mins, following the fast ice edge through mainly open water – the packing- in was occurring to the S. We did another CTD after 1 hr, seeing three large tabular Flade Isblink bergs within the pack, with clear visibility to the mountains and glaciers of Greenland behind. The CTD was at 79°40.17’N 14°16.48’W. After 90 mins of our run (in which swath bathymetry was done) we did a second CTD very near another large tabular berg which was grounded in open water. This was to see if melt water from the berg can be detected. Position was 79°44.58’N, 14°11.84’W, situated 0.25 ml from the berg. Water depth was 84 m. I took several photographs of the berg. We now ran back to the start point but found that more ice had packed in and we could now only get within 1.9 mls of recovery point. We put out hydrophone, hoping for best. The wind was still strong at force 7, snow whipping along, grey sky, like a typical winter ice edge. Wonder of wonders! At 1840, promptly, it replied. Saved! We all had dinner (of Indian food) then set out to recover it. Steve sent a message via hydrophone ordering the AUV to swim out to the position of the ship, which we had placed just outside the ice edge in an open water area, 2.54 nml from the AUV. Amazingly, the AUV responded straight away and swam obediently towards us, to come up a couple of hundred yards off our bow. What a relief! And what an achievement for the AUV team. The vehicle had reached right across Belgica Trough in deep water (500 m, uncharted), had avoided several obstacles, and had recorded a huge amount of data. Congratulations all round, relaxation in lounge then question of where to go next. I favoured southern entrance to Belgica Trough, but captain thought that way south was blocked by driven-in ice. So we went north towards northern entrance to Belgica Trough and area of North East Water Polynya (NEW). We coasted alongside the fast ice edge (widened by addition of pushed- in moving ice), occasionally having to come out to the E to avoid an iceberg and heavy pack ice. All seemed well. I left instructions, and so did the captain, that this was to continue, bringing us to Belgica Trough about breakfast time. Noon position 79°30.3’N, 14°12.8’W. AUGUST 23, MONDAY Heavy ice and poor visibility caused the ship to turn back. At 0600 we were only 10 miles north of where we had started. We immediately returned to a northward run, but we had lost many hours of work. The storm had gone, and we spent the morning heading north. I called Peter Lemke at 0830 about meeting plans. The ice soon eased and we made more rapid progress, coming round to the end of a northward peninsula which opened out to the W into the axis of Belgica Trough (or Dijmphna Sound), which appeared to be ice- free. Presumably the warm Atlantic water entering near the bottom was warming the surface. We decided to launch the AUV on the S side of the Sound and have it run into the ice on a 225° course, keeping slightly away from the Sound axis. We set it for a 12 hour mission. We would validate the ice conditions then do CTDs. Temporarily visibility was clear and we could see across to the coast.
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We launched the AUV just off the ice edge at 80°17.12’N, 13°00.82’W (mission 366). Then we ran into the ice (about 1500) and did a highly efficient ice profiling exercise, using 7 people (self, Jeremy, Nick, Zoe, Steve, Duncan, Guy). We did a 100 m line along the axis of the ship, a 100 m cross- line, two cores and five snow samples, all in two hours. What speeded things up was to have one person drilling with 1 m of flights and another following with a separate drill with 2 m of flights. The ice was relatively uniform first- year, between 1.2 and 1.5 m, thick. The small-scale variability in thickness will be a good test of how well the sonar resolves small depth variations. Then we pulled out, did a CTD, then ran NW at 330° doing CTDs at 5 mile intervals. We managed 4 in all, the last featuring heavy ice, which carried us across the deepest part of the Sound, about 340 m deep, and into slightly shallower water. Then we ran back to have a listen at the retrieval site in case the AUV had come back early (it is due back at 2.40 am). No sound. Noon position 80°11.3’N, 12°53.9’W. AUGUST 24, TUESDAY At 0030 we did a small excursion along 030° for 5 miles to do one more CTD (CTD15) while waiting for retrieval. We got back at 0240 and put down the hydrophone, The AUV responded immediately at a distance of 1 km. We guided it in to us (it lost lock once and went back to the 1 km mark) and brought it to the surface. The idea was to reprogramme it for an 8 hr run to flatten the battery, but the team found that the battery was already flat. Until we talked to Polarstern about the best location to meet we did not want to move significantly, so while the Autosub team started the 6 hour task of changing the battery packs we carried out some CTDs in the northern arm of the Belgica Trough.. The first took us 10 miles away on 030°. The next went on a further 5 n.ml. on 330° and took us back into heavy ice. We changed plans to return to a 330° line and do a station every 5 miles, a slanted run across the Belgica Trough. We did a line of 6 stations in all, leading to a Furthest North for the voyage of 80°38.74’N, 11°47.73’W, water depth 264 m. At 1000 I phoned Peter Lemke and we settled on 79°30’N as a place to rendezvous. Polarstern does not finish her other work until 0400 and does not have time to come far north, while we cannot get far south. So it is back to our original stamping ground. We will go there now, get set up, start running the AUV, and then they will join us with the helicopters and an 8-strong ice thickness team. We started making plans for validation and for a lawn- mowing AUV routine. The journey back involved crossings of some sunlit MIZs, sightings of bear tracks, and some beautiful calm vistas of the sun and clouds reflected in perfectly calm water. Then we got into tougher ic e and made slower progress. We passed four tabular icebergs recognisable from the journey north and plotted their positions. It was nearly midnight before we reached the fast ice edge at approximately the right latitude, then we had to coast south until there was enough of a slot of open water to seaward to launch and retrieve the AUV. Noon position 80°38.7’N, 11°47.6’W.
NERC Grant NER/T/S/2000/00985
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JR106 Cruise Report (v1.00)
AUGUST 25, WEDNESDAY We inserted ourselves into the fast ice edge at the intended location for the big experiment at 0015, at the position 79°20.56’N, 13°52.127’W. The ice appeared to be thick first-year or second- year ice with a network of well developed meltwater pools and some pressure ridging. One disadvantage is that a small berg 1.23 n.ml. inside the ice edge would be a barrier to deep penetration by Autosub, but we resolved that the best experiment would be a lawnmower survey of a 2 x 2 km experimental area (which would take 21 hours at 50 m line spacing) to cover validation work by ourselves and Polarstern, so the iceberg is not a problem. Steve drew up a plan for the survey, with 15 lines at right angles to the ice edge. Everyone got a small amount of sleep, then the ship was pulled out of the ice and Autosub was launched at 0600. The ship moved back in, breaking out a couple of segments of ice edge zone by the impact, and was firmly embedded in position for validation work. Meanwhile Polarstern was 24 miles away, heading towards us, having finished her line at 78°50’N, 10°W at 0400 We could not go out on the ice ourselves because we had no guns to defend against polar bears and the visibility was very low. A dense fog had descended at 0400 and looked unfortunately set to last all day, which it did. I talked to Lemke at 0800 and again at 1000. We arranged that they would come in and moor at the ice edge to the S of us (we were in the centre of the experimental box) and that we would share the calibration work, with them offering polar bear protection through three armed personnel. Just before noon a very vague shape loomed out of the fog and moored to the ice edge – coming alongside the edge rather than running into it – and lowered a gangway. After much discussion about polar bear protection, Polarstern ended up sending an armed escort the few hundred yards across the ice to us. I brought Steve Ackley with me, and we visited the ship where we had a session with Peter Lemke, Captain Donke and the sea ice scientists. We decided that one group from AWI would profile along lines of the survey with an EM system mounted in a hand-drawn kayak; one group would do resistivity measurements at an appropriate spot (Jim Bishop, formerly from Australia); and one would help us do drilling lines, especially by providing polar bear protection. This comprised Jan Leser, a sea ice meteorologist who is working on the SITHOS project. We headed back to James Clark Ross where Jeremy had already organised the ice squad to be ready for action. We laid out two 200 m lines in front of James Clark Ross running along the axis of the AUV survey lines, and a third line of 50 m across a distinct, though shallow, pressure ridge. The AWI kayak gang later covered both these lines and extended them to about 500 m, while Jim Bishop set up half way along line 1. The weather remained foggy and the helicopters could not fly, a real blow to the validation which we expected from the airborne EM system. We worked until 1800 and then Jan went off to escort a deputation from Polarstern across to our ship. We went back to James Clark Ross. The arriving group comprised Peter Lemke, Jan and four ships’ officers. We gave them a reception in the mess then dinner with wine. Straight afterwards everyone headed over to Polarstern for a party which they had set up on the afterdeck with glüwein. At the same time a big group from Polarstern wended their way across the ice to James Clark Ross for a party there. The groups disentangled themselves at 2200 when Polarstern was due to sail. There was some hope during the evening when the weather cleared and the helicopter took off with the EM system, but it NERC Grant NER/T/S/2000/00985
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came back after doing only one line, saying that the laser could not lock on because of the mist. Everyone thought it a great party, and we did not even see Polarstern leave, as the fog was so bad that she was invisible although only 500 m away. Noon position 79°19.5’N, 13°50.8’W. AUGUST 26, THURSDAY We sat in the ice through the early part of the night, hoping that the fog would clear enough to allow deployment of the Nagurny buoy on a pressure ridge which we saw some 250 m inland yesterday, but it did not. At 3 am we pulled out of our ice berth to retrieve Autosub, which was achieved swiftly and effectively thanks to the homing system, after a 21 hour mission (367). The weather is getting colder and a thin skim of nilas is now forming on the cold calm open water, especially because the fog is blocking out the sun. On surfacing Autosub was seen to be ploughing through this nilas like a semi-submerged icebreaker. Autosub was brought in because we believed that this was the last mission. The ship pushed back into the ice in her original position (but facing outwards) to allow us a final short experiment on the ice surface. We wanted to do a core, to establish the age of the ice in the survey zone, and to deploy the buoy. We were made wary by the sight of fresh polar bear tracks covering the beaten walkways developed by yesterday’s comings and goings, and also covering the floe edge beside yesterday’s mooring position. According to the deck crew, these had not been here at 3 am when we pulled out. Therefore we – that is, Jeremy, Duncan and myself – did the core right at the point where we were landed from the basket, and chose a smaller hummock near the ship (which had had the 50 m transect done on it yesterday) to be the site of the Nagurny buoy. This will probably mean that its lifetime will be short, but one can but hope. Back on board I received the serious news that the Autosub had only recorded data for the first third of the lawnmower survey, which did not include any of the survey lines run by ourselves or AWI yesterday. If we wanted to do something in the very short time still available there were only two alternatives – move the ship to the surveyed area and do a new line of holes, or relaunch the AUV and do a small number of lawnmower lines specifically to cover the survey lines. I hovered between the two, but was persuaded to go for the AUV by what happened next. One of the crew spotted three heads in the water in line, off the starboard beam. They looked like large ducks but it was soon clear that they were polar bears. I rushed up to the bridge and gave out the news. Immediately everyone rushed to look, deserting the bridge, and the sighting was piped over the PA system. Obligingly, the bears, comprising a mother and two cubs, hauled themselves out on a nearby ice floe, shook themselves, then started to gaze at the ship making sniffing movements with noses outstretched. Very likely it was the smell of bacon frying which attracted them – it made me hungry too. The ship drifted slowly back on them so that they were within a few yards of the stern, offering perfect photo opportunities for everyone. This of course slowed down preparations for the AUV launch, but it was not to be missed. Eventually the three bears plunged into the sea again and swam across to the main ice edge where they hauled out and ran swiftly away. Soon we saw the reason – a male bear
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pulled out on the floe which the mother and cubs had left. Obviously he was someone that they didn’t want to meet. He too sniffed the air, but plunged quickly back into the sea when we started to move forward and create turbulence from the stern. Very clearly this area is dangerous for surface operations, and we were very lucky not to be threatened yesterday. Steve now completed calculations for a 4- leg mini lawnmower covering our survey line, and the AUV was relaunched at 9.30 am. This was completed by 11.30, and after a nailbiting period when Autosub made a couple of homing runs which overshot, the vehicle was successfully recovered from mission 368 at 12.30, completing a highly successful series of missions on this cruise. We now began the journey home by extricating ourselves from the heavy polar pack which lay to seaward of us. Aided by Envisat images supplied by Richard Hall at NPI, we initially went north, then east and then gradually bore to the south. Noon position 79°20.1’N, 13°50.4’W. AUGUST 27, FRIDAY In the morning we began to cross the continental margin and came close to the 2500 m water depth required for a test of the SAMS Lander. A small deviation of course brought us to the 2500 m level on a shelving continental slope at 77°36.74’N, 4°07.08’W where we stopped. Duncan Mercer lowered the Lander, with its floats and chain weight, and tracked it acoustically as it sank to the seabed. Meanwhile the ship carried out a CTD, CTD20. With the Lander on the bottom we moved away 2000 m to see if tracking still worked. At this range it faded, but returned at 1500 m. With these tests complete, the signa l was sent to trip the release, and the Lander was then tracked as it rose to the surface, where it arrived after half an hour and was recovered. The ship then resumed her southward journey, continuing to collect swath bathymetry. The southward track is close enough to the outward track to allow overlapping parallel swaths. The Hardy- Longhurst continuous plankton recorder was streamed again as soon as we got under way, at 77°36.2’N, 4°06.4’W. In the evening I gave a talk on W.S. Bruce and the exploration of the Weddell Sea. Noon position 77°36.3’N, 4°6.7’W. AUGUST 28, SATURDAY We continued SW towards Iceland. The formal cruise dinner was held in the evening, followed by a party Plankton recorder cassette was changed. AUGUST 29, SUNDAY Final run- in towards Iceland, for arrival in Isafjordur on August 30.
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JR106 Cruise Report (v1.00)
AUTOSUB MISSION SUMMARY LOG Steve McPhail (Autosub)
360 361 362 363
364 365
366 367
368
Far WP
17/8 17/8 17/8 18/8 18/8 19/8 19/8 19/8 20/8
1843 2109 2142 0135 2215 0036 2000 2300 1345 2222
N:77:37.1, W:003 25.0 N:77:36.1, W:003 05.35 N:78:50.71, W:006:25.02 N:79 :17.22 W: 008: 31.1 N:79:30.0, W:014:20.5
N:78:52.71, W:006:34.52 N: 79 17.22 W 010 01.1 N:79:23.75 W:017:35.0
20/8 21/8 21/8 22/8
2356 0830 1840 2041
N:79:30.0, W:014:20.5 N:79:30.0, W:014:20.5
N:79:23.75 W:017:35.0 N:79:23.75 W:017:35.0
23/8 24/8 24/8 25/8
1426 0330 0602 0438
26/8 26/8
0920 1250
N:80:16.13, W:013:07.67 Corner 1 N:79:20.539 W:13:50.906 Corner 2 N:79:19.741 W:13:56.048 Corner 1 N:79:20.167 W:13:49.219 Corner 2 N:79:19.369 W:13:54.357
N:80:03.40 W:014:22.98 Corner 3 N:79:20.271 W:13:49.687 Corner 4 N:79:19.473 W:13:54.827 Corner 3 N:79:20.105 W:13:48.937 Corner 4 N:79:19.307 W:13:54.075
Comment Short shakedown test. Autosub had been programmed to surface if it did not receive an acoustic command within 40 minutes. Problems with the acoustic telemetry system prevented us doing this, and consequently Autosub surfaced after 40 minutes at the start waypoint. Position was off the continental shelf, hence no bottom track navigation. 3km run through 10% ice back to recovery position. No bottom track navigation. Homing Test. Autosub homed towards JCR at 1 km and 12 km range. No bottom track navigation. Head for 3 miles NW under ice flow, then back again. Bottom track navigation (and for all subsequent). Run underneath large ice flow and back again. For the first time the Em2k was configured with roll set to 0(as if looking downward). Run into pack ice. Intended 18 hr mission, but Autosub only ran for 7 hrs. It turned back because the collision avoidance was triggered due to limited depth of water. Same mission as 363. Autosub went a few miles into pack. Turned due to forward collision sensor sensing imminent collision. Ran for 24hrs into pack and back. Autosub collision avoided during return leg. Used homing system to aid recovery as the intended recovery waypoint had become covered with ice. Run 12 hours into pack. Completed successfully. Homing system was used to guide Autosub out from under pack ice for recovery. Lawn Mower run under fast ice at survey site. 50m track spacing. Run at 40m depth. Only 1/3 of mission completed successfully. Autosub appeared to have homed in the direction of the Polar Stern, possibly due to acoustic emissions from its survey systems. Homing started at 1232 on 24/8/04. Homing system used to aid recovery. Figure 1. Re run of section of survey mission 367 which had been planned to overlap with ground truthing and was missed due to the vehicle homing. Mission completed successfully. Figure 2. There is a moderate navigation anomaly between the dead reckoned position and the GPS fix at the end of the mission of 42 m east, 137 m north. The expected jump for this length of missions would be only +/- 20 m. The post processing software assumes, estimates and corrects for a constant velocity error between GPS fixes.
Navigation for Mission 366. LawnMower survey.
Mission 368 Navigation
79.349 79.36
79.344 79.35 79.339 Pos_N
359
Start Position N:77:37.1, W:003:35.0
Pos_N
358
Date Start/ End 17/8 0942 17/8 1030
79.34
79.334 79.33 79.329
79.32 79.324 -13.94
-13.92
-13.90
-13.88
-13.86
-13.84
-13.82
-13.80
Pos_E
Figure 1: Navigation for Mission 367. Survey was interrupted by Autosub entering homing mode at 1232 on 24/8/04.
NERC Grant NER/T/S/2000/00985
-13.91 -13.90 -13.89 -13.88 -13.87
-13.86 -13.85
-13.84 -13.83 -13.82 -13.81
Pos_E
Figure 2: Navigation for Mission 368. Post processing assumes a constant velocity error between GPS fixes. This causes some distortion to the apparent track.
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JR106 Cruise Report (v1.00)
AUTOSUB NAVIGATION SYSTEM PERFORMANCE Steve McPhail One of the pre-cruise concerns was how would the Inertial Navigation System (IXSEA PHINS, Fibre Optic Gyro based) cope with the high latitudes. INS systems generally perform less well at higher latitudes, both in terms of accuracy, and the time they take to align following power up. The alignment issue was quickly resolved. Even at 80ºN, the INS settled within 10 minutes of power up. The accuracy of the combined navigation system, when aided by ADCP bottom tracking is examined in Table 1. The missions without bottom tracking are not included in the analysis. The errors given are the difference between the dead reckoned position and the GPS fix at the end of the mission.
Mission
Latitude deg N
North Error (m) East Error (m) Radial Error (m) Distance Travelle d (km)
Error % of distance travelled . Dive Weight Dive ?
Table 1. Navigation accuracy for Autosub. Missions 361 to 368.
36 1 36 2 36 3 36 4 36 5 36 6 36 7 36 8
78.5
-7
-34
36
11.0
0.32
Y
79.3
55
2
55
13.3
0.42
Y
79.5
-26
-6
28
42.1
0.066
N
79.5
162
-110
195
22.2
0.86
N
79.5
111
-24
114
145
0.079
N
80.3
145
-193
242
80.28
0.30
N
79.3
-64.7
-7.6
65
73.5
0.089
Y
79.3
137
-32.1
140
14.9
0.93
Y
At first sight these results are a little perplexing. The results appear to fall into two groups either very good (average 0.08% of distance travelled), or rather mediocre (average 0.6% distance travelled). The accuracy does not seem to correlate with latitude, whether the mission is long or short, or whether a dive weight or surface run is used. ADCP data for the “bad” navigation run, show no obvious proble m. The ADCP mode remains fixed at ‘0’, (bottom track) throughout the mission, and there is no apparent missing ADCP data. Another possible cause is GPS outages. On Mission 368, a jump of 80 m in GPS position at the start of the mission is indicates that there may be a problem with GPS jumps.
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JR106 Cruise Report (v1.00)
AUTOSUB COLLISION AVOIDANCE Several of the JR106 missions where carried out in conditions where there was limited headroom between the seabed below and the under ice surface above. In such conditions the operation of the collision avoidance system on Autosub was critical. The collision avoidance system takes sensor data from the upward and downward looking ADCP ranges, and from a single beam echo sounder pointing forward. The system is triggered when either of two conditions occur: The safe lower depth limit (set by minimum altitude, or maximum allowed depth settings) and the upper depth limit (set by minimum range to the base of the ice or minimum depth setting) overlap. For example if the Autosub minimum altitude is set to 30m, and the minimum depth is 40 m, then the collision avoidance is triggered if the water depth falls below 70m. A 120 kHz echo sounder, pointing forward registers a target with continuous decreasing range, for 10 seconds (configurable), and less than a critical range of 100 m (also configurable). The challenge is in adjusting the operating parameters (e.g. minimum altitude, minimum depth and the time / range settings for the forward echo sounder) in an attempt to make the system sufficiently robust against false triggering, while responding to real threats. The behaviour of the vehicle following triggering of the collision avoidance state, is configurable. In most cases, when an obstacle is encountered when the Autosub is heading out, we configured it to abandon the mission and head back towards the recovery waypoint. This occurred on missions 363 (due to limited headroom), and for mission 364 (due to collision imminent sensed by the forward echo sounder). Following this we reduced the minimum altitude to 25 m and set the Autosub off on a long 24 hour under ice (mission 365). On this occasion the Autosub was able to get to the destination waypoint, but detected an imminent collision on the way back. In this situation, Autosub attempts to find a way around the hazard, by first retreating along is path (known to be safe), and then attempts to round the hazard by trying a different track. If it encounters the obstacle again, it repeats this behaviour but with a randomly chosen new track. Figure 1 shows that it took three attempts for Autosub to find its way around the obstacle. Figure 1. Track and depth of Autosub as it manoeuvred around an obstacle detected by the forward looking sonar, during the return leg of mission 365. The Autosub track is from left to right (heading Eastwards). It turns around twice and retreats, finally succeeding in avoidaing the hazard on the third attempt.
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Analysis of the engineering data showed that during the first approach to the obstacle, the Autosub control system did not react to the first occasion that the obstacle was detected. This was due to loss of one “collision imminent” message on the control network. Following this, we changed the protocol for the message passing for this message from unacknowledged to acknowledged, making a repeat of such an occurrence extremely unlikely.
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AUTOSUB HOMING SYSTEM AND ACOUSTIC TRACKING Homing System There were two tests of the homing system before it was used in anger. On M359 the sub was successfully made to home from a range of 13.2km, and it then returned to its preprogrammed recovery waypoint ten minutes after homing ceased. On M360 the sub was successfully called tot he ship and circled several times at a range of less than 100m for more than 90% of the time. Below, the green portion of the otherwise blue track shows the position of the sub in homing mode and the black portion of the red track shows the position of the ship at the same time. Apart from one excursion to 300m the sub heard the homing
signal within 100m of the ship and turned back towards the ship after passing it. All passes were within 50m and the three were within 10m, the closest being about 3m. Both of these missions were in a water depth of 3000m. It was noted that the sub received the homing signal more readily when heading towards the ship than away from it, as expected from the position of the receiver array. Most of the operational homing was carried out in a water depth of 100m-160m: M363: The sub’s recovery position was under and ice floe, and it was called to the ship and given the surface command from a range of 500m. M365: The pack ice moved in to cover the recovery position and the sub was called to the ship from a distance of just over 3.9km M366-368: On these occasions the sub’s recovery waypoint was considered unsafe. The ship was moved to open water 300m-800m away and the homing signal was used to call the sub to us. The mission script was altered so that the sub would circle up to the surface on command, enabling it to be surfaced 200m-300m from the ship. On M367 the thickness of fresh sea ice was such that it was detected by the sub, which stayed circling at 30m until the “surface” command was used to override this. Also on M367, the sub received several false homing commands. These appeared to emanate from the R.V. “Polarstern”, which was stationary alongside the sea- ice for several hours. It is likely that they were transmitting with a chirp profiler which was interpreted incorrectly by the homing system.
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Deploying and recovering the homing transducer array from the ship with 45m of cable was made easier by the use of a roller clamped to the rail, provided by the boatswain. The emergency beacon was set to transmit every ten minutes. This was used to detect the approach of the vehicle before the acoustic tracking could pick it up, and usable ranges were obtained out to 9km slant range. On more than one occasion the sub returned early due to the obstacle avoidance being activated, and listening for the emergency beacon meant tha t its approach was detected and it could be recovered or reprogrammed with the minimum waste of time. Acoustic Tracking and communications The primary acoustic tracking system, the ORE Trackpoint-2, did not function and had to be replaced with the backup system, the LXT. The LXT transducer was successfully mounted on the tow-fish but the plotting program, the IPS, did not always plot the transponder replies. The stability and accuracy of the LXT, however, meant that using the raw data to get the sub’s range and bearing was straightforward. Usable ranges of up to 4.5km with the sub approaching the ship were obtained in 160m of water, but reliable ranging was generally at 2km or less. It was not generally possible to steam with the tow- fish deployed because of the danger of snagging the cable on sea- ice. The Applied Acoustic digital acoustic link was used over ranges of 500m or less, and worked as well as it had done on the most recent trials cruises.
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AUTOSUB MECHANICAL REPORT Steve McPhail and Andy Webb (Autosub) Mobilisation Autosub mobilisation began at Portland in July following the ship’s refit and sea trials and prior to cruise 105. At this time the launch and recovery gantry was bolted to the deck matrix, the aft container secured in place with its roof extension raised and the Autosub vehicle secured in its container. This work enabled the completion of mobilisation at Reykjavik (fixing the second container and installation of forward acoustic fish, installation of computer and aerial systems) to finish ahead of schedule. The layout on the aft deck was the same as the previous AUI campaign in 2003 (JR 84). Figure 1 shows a plan view of gantry and Autosub’s purpose made containers on the aft deck.
Figure 1 Plan layout of the containers on the aft deck
Vehicle configuration Figure 2 is a schematic showing the basic vehicle layout, Table 2 is the relative positions of the sensors on board, with respect the vehicle datum (the bottom of the forward bulkhead joint, see Figure 2).
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Figure 2. Vehicle layout showing sensor space and datum.
Sensor
CTD (port and starboard)
Longitudinal centre of gravity wrt vehicle datum (m) -1.1
Vertical centre of gravity wrt vehicle datum (m) 0.45
Oxygen sensor
-0.57
0.45
Digiquartz Depth sensor EM 2000 Transmitter EM 2000 Receiver 300kHz ADCP
-0.5
0.65
-0.65
0.8
3.87
0.7
3.33
0.85
150kHz ADCP
3.45
0.1
Forward looking echo sounder Camera Camera flash
-0.14
0.45
4.0 -0.97
NA NA
Aqualab water monitor
Remarks
Ports side, Temp1, Ser No. 03P2342. Cond1 Ser No. 2730 Starboard side, Temp 2 Ser No. 03P2912. Cond2 Ser No. 2760 Plumbed in the starboard side with Temp2 and Cond2
Position of transducer head looking upwards Position of transducer head looking upwards Position of transducer heads looking upwards Position of transducer heads looking downwards Position of transducer head looking forwards
Tilted to illuminate spot beneath camera at 10m -0.69 0.55 Position of sampling ports (Not used for Leg 1of the cruise) Table 2. Positions of sensors relative to vehicle datum.
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Operations The ballast and trim of Autosub has to be carefully tailored for the local conditions to be 8 to 12kg buoyant and neutral trim in order for it to both float and control without difficulty. Sea water density measurements were made using water from the sea water supply in the Wet Lab and a floating hydrometer. The Autosub vehicle was floated in Reykjavik harbour with lines attached as a check that no significant change in weight had occurred as a result of the battery change made at the SOC. The water density and vehicle weight estimates indicated a buoyancy of 18kg. The vehicle just floated (circa2kg buoyancy) when floated with 13.5kg of ballast taped on top, indicating the estimates were sufficiently accurate. Table 1 shows the history of the density measurements and the changes made to the vehicles ballast and trim throughout the campaign. Autosub started the leg with fresh batteries and underwent two battery changes throughout the science time. The battery packs were from two suppliers, A1 Marketing Ltd, Bordon, Hants (Rayovac cells), and Steatite Ltd, Redditch, (Fujitsu cells). In addition to the problems of variable weights between the two sorts, there is evidence of the Fujitsu cells having less capacity than the Rayovac cells. The Autosub team will investigate this further. The vehicle performed well with few faults. The mechanical problems encountered were:• • • • •
1 abort weight jettisoned unnecessarily (network problems) 1 sink weight dropping off the safety pressure release (tolerance problem on the design of the dive weight) Intermittent sternplane servo positioning problems (traced to a dry soldered joint on the feedback potentiometer). Sluggish performance of the launch and recovery gantry in icy conditions Intermittent braking problems on the rotary carriage drive on the launch and recovery gantry (to be investigated by the Autosub team at a later date)
The vehicle needed no repairs beyond normal maintenance of:• • • • • •
Battery changes Flushing of CTDs Cleaning and re- greasing propulsion motor bearings Recovery line stuffing Packing the “Jack in the Box” grappling line Adjustments to ballast and trim
The major consumables used were:• 3 battery sets (28 packs/set). Some usable life still remains for the trials on the following leg. • 1 Abort weight • 7 sink weights (one dropped in error)
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JR106 Cruise Report (v1.00)
Date
Time
Location
Water Density (kg/m3 )
12/08/04
-
Reykjavik harbour
1027 (16C)
17/08/04
-
Prior to mission 358
18/08/04
20:30
Prior to mission 361
19/08/04
-
21/08/04
17:15
23/08/04
-
24/08/04
13:00
1) 2)
Changes made to Autosub ballast No change
Changes made to Autosub trim No change
1025.5 (1.4C)
No change (see note 1)
No change
1025.5
1kg removed
No change
1026
No change
Prior to mission 365
1026
13.4kg added
+1.4kg.m (nose up) -2.3kg.m (nose down) see note 2
Prior to mission 366 Prior to mission 367
1025.5
-
No change
+2.3kg.m (nose up)
9kg removed
No change
Remarks
Judged to be 2kg buoyant with 13.6kg lead ballast added Very calm conditions with potentially very little mixing of fresh melt water on the surface. Vehicle appeared only marginally buoyant and slightly nose down after mission. -
1st battery change (2nd pack), the fresh battery packs were 13.4kg lighter than the 1st pack. Trim error corrected to make vehicle neutral again. 2nd battery change (3rd pack), batteries 4.3kg lighter than the 1st pack
The water temperature of 16C compared with 1.4C temp causes an estimated contraction of the foam and pressure vessels (the main sources of buoyancy) of 0.7 litre Made in error, trim should have been left without any change.
Table 1. History of trim and ballast changes
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AUTOSUB SCIENTIFIC SENSORS For JR106 the Autosub vehicle was fitted with the following scientific sensors: • • • •
RDI 150kHz ADCP looking downwards RDI 300kHz ADCP looking upwards Kongsberg EM2000 Multibeam swath system looking upwards. Seabird 911 CTD system.
In addition an Edgetech sub-bottom profiler was also fitted but not used on this cruise. These instruments are described separately in the following sections. Table 2 in the Autosub Mechanical section of this report shows the exact sensor locations. All the electronic systems on the vehicle are connected to a single control network. The data from all sensors apart from the multibeam system are recorded on the Autosub data logger. The Autosub logger uses a proprietary data format but the data is translated into standard ASCII text files using the Logger File Translator software running on a PC. This software also translates the CTD data into a standard Seabird format file. The resultant ASCII file is then imported into the Axum processing software and a standard script is run to produce the general post processed navigation file (.bnv file) and various instrument specific files including a navigation file for the EM2000 multibeam system. Sensor Synchronisation. The time synchronisation of the various on-board systems is important, especially where data from different systems is likely to be merged at a later date (post processed navigation data for the EM2000 is one example of this). Wherever possible the network time protocol (NTP) system is used which allows for time comparisons with a resolution of better than 1millisecond. The primary reference is a GPS receiver which sends an accurate pulse on each second boundary to the Autosub shipboard data server. The Edgetech sub-bottom profiler acts as the primary Autosub vehicle time server and uses the Autosub shipboard server as a reference whenever Autosub is in contact with the ship. The Autosub logger can synchronise to the Edgetech on start up and the Kongsberg EM2000 is synchronised to the logger. One problem is the poor quality of the logger clock which can drift by 10 seconds in 12 hours. The data processing system can measure and compensate for this drift so that the data output in the navigation files is correct. However, in the case of the EM2000, it was realised towards the end of the cruise that the raw time must be used for the post processed position timestamps rather than the drift compensated position. A revised version of the logger file translator software (V2.90.06) was produced which outputs both raw and compensated time but, due to time constraints, the post processed navigation files intended for use with the EM2000 will have to be re-processed after the cruise using a revised data processing script (JR106WithHomingAndEM2kNavV2.axs). The Autosub TimeSync monitoring software is run during each mission in order to monitor the clock drift between underwater systems and various shipboard systems. The results are stored in the TimeSync directory. The .txt file is the more verbose version while the .dit file contains the differences in an ASCII table which can be read by most data processing software.
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Seabird 911 CTD system. Autosub is fitted with a Seabird 911 CTD system which includes two sets of conductivity and temperature sensors. These are mounted in a ducted system with sea water pumped through them at a precisely known rate. Depth is measured by a Digiquartz pressure sensor. In addition, a Seabird SBE 43 oxygen sensor is fitted which is situated in the same duct as the secondary CT sensors. The output from these sensors is recorded at a rate of 24Hz. Sensor Primary Te mperature Primary Conductivity Secondary Temperature Secondary Conductivity Oxygen
Location Serial Number Port Side 2342 Port Side 2730 Starboard Side 2912 Starboard Side 2760 Starboard Side 0259
Data from the system is continuously logged whenever Autosub is switched on but, in order to prevent excessive wear on the pump, water is only pumped through the C/T sensors once a predetermined pressure threshold has been exceeded. The data is stored on the Autosub logger in a proprietary format but is normally translated into a Seabird format data file (.dat) at the end of each mission. This data file, together with the necessary configuration file was then passed to the scientific party for further processing. Sensor calibration data is stored in a separate file with the .con extension. For the JR106 cruise the data was initially processed using the 0696Plym04bPre.con file which contained the most recent calibration data prior to the start of the cruise. An unprocessed section of the data from mission 361 is shown below. This appears to show a good correlation between the primary and secondary sensors although the secondary temperature sensor (the blue line) appears more noisy. This data would normally be further processed to compensate for the time delay between T and C sensors in order to remove any false salinity spikes. 2.70
2.69
-1.1
-1.1
2.69
2.68
-1.2
-1.2
2.68
2.67
-1.3
-1.3
2.67
-1.4
-1.4
-1.5
-1.5
-1.6
-1.6
2.63
-1.7
-1.7
2.63
2.62
-1.8
-1.8
2.62
2.61
-1.9
-1.9
2.61
2.60
-2.0 4500
-2.0 4750
2.60
2.66
2.65
2.64
Temperature [ITS-90, deg C]
-1.0
4525
4550
4575
4600 4625 4650 Time, Elapsed [seconds]
4675
4700
4725
2.66
2.65
2.64
Conductivity, 2 [S/m]
-1.0
Temperature, 2 [ITS-90, deg C]
Conductivity [S/m]
m361.cnv 2.70
Figure 1. Primary and Secondary Conductivity and Temperature Data for a Section of Mission 361
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However, towards the end of the cruise it was noticed that the data from the SBE 43 Oxygen sensor was not giving sensible results. On further investigation in appears that the sensor had been connected to analogue input 4 rather than input 0. A new configuration file, 0696JR106Start.con, was produced which will accept oxygen data on analogue channel 4. The oxygen sensor data for the same period as figure 1 is shown below in figure 2. m361.cnv 2.70
2.70
4.50 8.0
2.69
2.69 4.25 7.5
2.68
2.68 4.00
7.0
2.67
2.67
Oxygen, SBE 43 [ml/l]
Conductivity [S/m]
2.64
3.50
6.0
5.5
3.25
5.0
3.00
2.63
2.66
2.65
2.64
Conductivity, 2 [S/m]
2.65
6.5
Oxygen Voltage, SBE 43
3.75 2.66
2.63
2.62
2.62 4.5
2.75
2.61
2.61 4.0 2.50
2.60
2.60 4500
4525
4550
4575
4600 4625 4650 Time, Elapsed [seconds]
4675
4700
4725
4750
Figure 2. Oxygen and Conductivity Data for a Section of Mission 361
Some of the sensor calibrations are now rather old and it would be advisable to have these sensors re-calibrated when the equipment is returned.
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JR106 Cruise Report (v1.00)
AUTOSUB - KONGSBERG EM2000 MULTIBEAM SWATH SYSTEM The Kongsberg EM2000 is a multibeam swath bathymetry system which operates at a frequency of 200kHz and can give up to 111 beams of data with an angular coverage of up to +/-60 degrees under favourable conditions. On Autosub the instrument is triggered by a controller connected to the vehicle’s LONWorks network. This controls the ping rate and also allows the trigger pulse to be synchronised with other systems on the ve hicle in order to control interactions between instruments. This controller also sends time and navigation information to the instrument. A recent software update to the EM2000 now allows it to receive range aiding data from this controller. This range aiding, which gives the distance from the seabed or from the surface as appropriate, seems to have improved the data quality from the instrument. A second LONWorks controller sends attitude and depth information to the instrument. For JR106 this system was fitted with the transmit transducer mounted in the nose of the Autosub vehicle and the receive transducer was mounted in the tail section facing upwards. The transducers were mounted behind polythene windows in the vehicle’s fibreglass outer panels (See table 2 in the Mechanical section of this report for exact sensor locations). The initial instrument settings used were those that appeared to have given good results on the recent Plym04b trials cruise. The EM2000 rejects any data that appears to come from above the sea surface. When looking upwards it is possible that legitimate data may appear to be above the mean surface level so a depth sensor offset of –1.5metres was introduced to counteract this. The beam spacing was set to be equidistant and the maximum beam angles were +/- 60 degrees. The first mission to give data from the EM2000 was mission 359 which was run in reasonably open water with a few well spaced ice floes. A short section is shown below in Figure 1. There appear to be returns from the ice but the sea surface does not appear to have been properly detected as the outer beams show increasing depths rather than a flat sea surface and, given the depth sensor offset, the sea surface should be at a greater depth than found in this data. Two factors were identified which could have caused this; a) the instrument sound speed was set to 1500ms-1 while the true sound speed was closer to 1450ms-1 and b) the depth sensor offset may have been too low. Both of these factors would cause the sea surface to appear to be above zero.
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Figure 1. Section of Gridded EM2000 data from Autosub Mission 359
The next mission suitable for running the EM2000 was mission 361 where the depth sensor offset was increased to 2.5m. An attempt was also made to change the sound speed used by the instrument but it appears that, although the speed appeared to have been updated in standby mode, the instrument actually retained the 1500ms -1 setting when pinging. The upwards looking ADCP had appeared to only see the sea surface intermittently on mission 359 so the source of the depth aiding information was also changed from the upwards looking ADCP to the depth sensor. This time the instrument did appear to see the sea surface in the vertical centre beams but the increasing depth at the outer beams remained. In open water the centre beams showed consistent depths of around 0.3m when Autosub was running at a depth of 30m and 0.6m when running at 40m. The change in centre depth is approximately 3% of the depth difference which could be consistent with the incorrect sound speed setting which was 3.4% higher than it should have been but this should have resulted in the surface appearing to be further away with increasing vehicle depth. This has not yet been satisfactorily explained. After further investigation it appears that any sea surface reflections in the outer beams are being swamped by the extremely strong vertical reflection which results in the apparently curved sea surface. The sea conditions were very calm during this mission, as they were for most of the cruise, which could explain the poor returns obtained from the outer beams. In order to ensure that no data which appeared to be above the surface was discarded it was decided to change the sensor roll settings to make the instrument appear to be looking downwards. The S1R and S2R parameters in the install file were set to zero. This also removed the need for the depth sensor offset which was now also set to zero. This change has very major implications for the data processing as the Kongsberg supplied software will no longer be able to handle this data properly. In this configuration the port and starboard sides are reversed and the pitch angle must also be inverted before the data can be used.
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Mission 362 and all later missions were run in this configuration. While, from an engineering point of view, the system appeared to be collecting data, it will not be possible to look at the data in any real detail until suitable processing software has been written. The plot below highlights some of the problems that have still to be addressed by the additional processing software.
Figure 2. Section of Gridded EM2000 data from Autosub Mission 368 showing anomalies due to deliberate false roll setting.
The edge of the fast ice can be clearly seen but there are discontinuities between adjacent beams caused by the port/starboard reversal and the deeper depths shown by the red sections are caused by the vertical echo swamping the sea surface returns where no ice is present. The Autosub tracks shown in this diagram come from Autosub’s internal navigation system. This navigation data can be greatly improved by post processing using GPS information at the start and end of the mission. Kongsberg have supplied the Hugin2Survey software which can accept a post processed navigation file and incorporate this information into their gridded data format. Any additional processing must also have the ability to import this navigation data. Towards the end of the cruise Kongsberg emailed an update to the EM2000 DSP code to improve vertical surface echo rejection in the outer beams but this was not used on the cruise as Kongsberg had not had the opportunity to fully test it and it would have required us to run a number of test missions with different rejection settings in order to ensure that it improved the vertical echo rejection while not impairing the under ice imaging.
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The upward-looking EM2000 multibeam sonar tunnel roof artefact Arthur Kaletzky (DAMTP) The AUV was launched for the first time on this cruise on ......... at position ....... . Among the data resulting from this mission were several EM2000 upward looking sonar “raw” (actually, semiprocessed for virtual beam forming and edge detection, since the EM2000 cannot output raw stave data) data files. The run was conducted in very still, largely open water with some ice floes. The plots resulting from further processing of these data were surprising. Most scans depicted a curve symmetric around the zenith of the AUV in the vertical plane containing its roll axis. The curve descended sharply and symmetrically on each side of the zenith and was first thought to be a parabola, for which there was no apparent physical explanation. However, when the plot axes were made of equal scale, it was seen to be a circular arc (it was actually an arc of an ellipse when z was exaggerated as customary). The immediate hypothesis arose that all of the virtual beams were somehow being polluted by a strong and sharp omni-directional ping. Software was written to examine the “raw” depth and “raw range” datagrams in the “raw” files and it was found that actually the strength of the reflected signal dropped off rapidly with increasing angle between the virtual beam and the AUV zenith, but was nevertheless sufficient to dominate all other returns in most virtual beams and thus be detected by the EM2000 embedded software as the defining edge of the imaged object - thus the circular arc, which when the successive scans were put together formed the “cylindrical tunnel roof” artefact. In some but not most scans, there were beams which contained reflections stronger that the “roof”, and then the correct images of the reflecting objects were formed. By comparing these and later mission data, it was seen that the artefact was most prominent when there was very still water rather than rougher water or ice overhead the AUV. The obvious conclusion was reached - the specular reflection from overhead still water is so strong that it leaks into virtual beams pointing in other directions. The virtual beams, just like the physical stave beams from whose data they are derived, are not perfect they have side lobes with greatly reduced but nonzero transfer functions. Because multibeam sonar unlike electromagnetic radar depends on a multidirectional source with all reflections of a scan being caused by a single multidirectional ping, a very strong reflection (several orders of magnitude greater than any other in the scan) can leak into other beams through their side lobes creating the tunnel roof artefact. This artefact can be fairly easily recognised and removed using specially- written postprocessing software which we are now developing. However, because the EM2000 does edge detection onboard using proprietary embedded software which deletes all reflection data not near the “detected edge”, we cannot replace the deleted reflections with more credible ones. Thus, until we can deal with this problem with the manufacturer, we must simply reject scans where this artefact occurs, all scans with still water rather than ice or rough water overhead. We have contacted the manufacturer and received an onboard software patch from them by Inmarsat e- mail. However, we decided not to apply the patch on this cruise because of schedule risk (there were only 2 more mission days available when the patch was received) and good ice cover which prevented the artefact from appearing.
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JR106 Cruise Report (v1.00)
AUTOSUB POST-PROCESSED NAVIGATION DATA FORMAT Steve McPhail Post processed navigation data is provided in a file Mxxx.bnv, where xxx is the mission number. The file is ASCII text with comma separators. The first line is the column headers. Missing data is represented by “–999”. The frequency of data output is once every 2 seconds. Field Date Time Seconds Elapsedtime Pos_E Pos_N Depth Vel_E Vel_N PosRaw_E PosRaw_N PosError Posfix_E Posfix_N FixType TSLF ADCPVelMode LineIndex ADCPVel_E ADCPVel_N ADCPAlt Driftrate_E Driftrate_N Travelled_km LPVel_E LPVel_N Vwater_E Vwater_N WaterSpeed LPGroundSpeed LPWaterSpeed Pitchdeg Headingdeg Rolldeg Splanedeg Rudderdeg prop_rpm WaterDepth MissionNum MCLongDem MCLatDem_ Total Power battery_V
Table 1. Data Field Definition Table Units Description m/d/yr mm:dd:yy Julian Data. hr/mn/s hh:mm:ss. UTC s Seconds Since 00:00:00 1/1/1970 s Since start of navigation file. degrees “Best estimate” Longitude. degrees “Best estimate” Latitude. m Depth of vehicle. ms -1 “Best estimate” East Velocity component. -1 ms “Best estimate” North Velocity component. degrees Raw (unprocessed) Longitude. degrees Raw (unprocessed) Latitude. m Estimate of the position error. degrees GPS Fix: longitude degrees GPS Fix: latitude enumeration GPS fix type. 2 (D),3 (3 D),4 (2 D diff.), or 5 (3 D diff). s Time since the last accepted GPS fix. enumeration ADCP mode of operation: 0,1,2 Integer Mission Line number. ms -1 East Velocity output by Autosub ADCP. ms -1 North Velocity output by Autosub ADCP. m Altitude measured by ADCP. ms -1 North Drift rate (or current) estimate. ms -1 East Drift rate (or current) estimate. km Distance traveled (over ground) in km. -1 ms North component Low pass filtered velocity. ms -1 East component Low pass filtered velocity. ms -1 North velocity through water. ms -1 East velocity though water. ms -1 Speed through water. ms -1 Ground speed. Low pass filtered. ms -1 Through water speed. Low pass filtered. degrees Pitch of vehicle (degrees) degrees Heading of vehicle (degrees) degrees Roll of vehicle (degrees). degrees Stern Plane degrees degrees Rudder degrees Rev per Propeller Radial Speed minute m Depth of water. Is Depth + ADCPAlt REAL Mission Number: +Number at Start of Mission. - Number at the end of the mission. degrees Longitude and Latitude Demands from Mission Control. Effectively are the mission waypoints. Watts Total electrical power usage. Volts Battery Voltage.
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AUTOSUB ADCP DATA DEFINITION (JR106) Steve McPhail Physical Arrangement Autosub has two RDI ADCPs: A 300 kHz RDI Workhorse pointing upwards. A 150 kHz RDI Workhorse pointing downwards. Both can provide velocities in bottom tracking mode (or ice tracking for the upward looking ADCP), as well as current profiling. The range information for the four beams is also used in the control of the vehicle, where it is set to keep a constant distance from the seafloor, or under the ice. The collision avoidance system also takes input from the ADCP beam ranges. Approximate performances seen during JR106 are: Up ADCP. Ice tracking 100 to 200m. Water profiling to 80 m (typical) Down ADCP. Bottom tracking to 450 m range. Water profiling to 144 m (typical). Both are currently set with 8m profiling bins. This can be changed, although shorter bins will give higher noise values (particularly for the down looking 150 kHz), and it would complicate processing to have different up and down bin lengths. Files: The ADCP data is contained within the ASCII mxxx.ls2 files, where xxx is the mission number. The first line of this file is a header of field names). The second line are the units used. The data is 2 seconds sorted (new set of data each 2 seconds). This file also contains Autosub engineering and (unprocessed) navigation data, some of which might be of interest. For post processed (more accurate) navigation data, you might want to use the Mxxx.bnv (best navigation) file which is described in a separately. Where there is no data within a 2 second period the missing data value is represented by –999. The ADCPs produce new data every 2.6 seconds. This explains why, in the 2 second binned data file (ls2), there are regular missing data values (-999). The ADCPs themselves use –32678 to represent no or bad data.
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ADCP Data Fields in the Mxx.ls2 files Table 1. ADCPbin[0] Frame 0 is a special frame with ADCP configuration data Field Name UNIT Description CellIdx0* 0.24 dB ADCP beam 3 intensity for bottom target Inten0* 0.24 dB ADCP beam 1 intensity for bottom target Veast0 mm/s Starboard velocity relative to seabed Vnorth0 mm/s Forward velocity relative to seabed Vdown0 mm/s Down velocity relative to seabed Verr0 mm/s Error velocity ADCPVersion RDI firmware version and revision ADCPRev HeadingBias 0.01 deg Always set to 0. Number of Water Pings Number of water pings per ensemble. Usually set to 1. Size of cell Cm Vertical length of profile cell in cm. Blank after TX Cm Blanking distance. 1st bin begins after this. Number of Cells Number of profiling bins. Up to 48. Minimum Threshold 64 usually Heading Align 0.01 deg 4500 for the down. –4500 for the up. The ADCPs heading axis are rotated 45 degrees relative to the vehicle. Salinity User set Salinity used in velocity calculation. Eg. 35 SoundSpeed m/s Calculated by ADCP based on Salinity (fixed), temperature (measured in ADCP and, and depth (externally measured). ADCPTemp (0.1 ADCP measured temperature. Celsius) Table 2. ADCP water profiling data bins[1 to N]. Example shown for the first bin (index 1) Field Name UNIT Description CellIdx1* 0.24 dB ADCP beam 3 intensity. Inten1* 0.24 dB ADCP beam 1 intensity. Veast1 mm/s Water profile velocities are in levelled ship frame of reference, relative to the PHINS forward axis. Vnorth1 mm/s starboard, forward, down, and error. Vdown1 mm/s Verr1 mm/s
For the Upward looking ADCP, the fie ld names have ‘_2’ appended.
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Table 3. Other Data fields in the ls2 files which are of interest to users of ADCP data
Field Name Date Time Seconds Roll Pitch Heading
Units e.g.17/08/2004 e.g. 09:40:02 e.g. 1092735602.0000 Radians Radians Radians
Description Date Time of day (UTC) Seconds since 1/1/1970
Roll angle of Autosub. (+ve to starboard). Pitch angle. +ve node up. Heading. In Navigation convention. Heading north is 0. East is pi/2. INSLat Degrees (decimal) Latitude (not post-processed) INSLong Degrees (decimal) Longitude (not post-processed) INSDepth Metres Depth of Autosub (m). * There is a bug in our logging software, which causes the intensity values to “wrap around” for values greater than 127. The correction, easily applied in Matlab is : // for all val.. if(val <0); val = val+256; end; Hints for processing the ADCP data You’ll only get good current data when the down ADCP has bottom track. Processing steps: Transform “Ship Levelled” to geographical. e.g. Vnorth = Vfwd*cos(heading) -Vstbd*sin(heading) Veast = Vfwd*sin(heading)+ Vstbd*cos(heading). (In the ls2 file : Vfwd is called Vnorth , Vstbd is called Veast). Produce Current profiles from the vector equation. Vwater(geog) = Vbottomtrack(geog)+ Vcurrent(geog). Map the current profiles to real depths, by adding on the Depth sensor reading to the profile depths (based on bin size, bin number, blanking distance).
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JR106 Cruise Report (v1.00)
SEA ICE VALIDATION PROGRAMME Peter Wadhams Drilling When AUV transects were carried out under fast ice, the primary means of validation consisted of lines of holes drilled through the ice near to the ship (which was forced into the ice edge) and oriented along and over a known track of the AUV. The procedure was as follows: A start point, marked by a flag, was defined by portable GPS as lying over an Autosub track line. A 100 m line was laid out in the direction of the AUV transit, marked at 50 m intervals. Holes were drilled at 5 m intervals using a petrol-driven power head and a CRREL 2-inch augur. Measurements were made of: snow thickness at three points near the hole; total ice thickness using a scissor-type probe; and ice freeboard. Features such as melt pools along or near the track were noted. A 100 m cross- line was then surveyed starting from the centre of the primary line and the survey repeated. If time permitted, the primary line was extended to 200 m. Finally, snow samples were taken with a standard sampler to obtain snow density measurements. Results are given in Appendix A. Coring Ice cores were taken from at least two locations in each survey area, using a CRREL 4-inch corer supplied by Kovacs Instruments. The cores were stored temporarily in the ship’s deep freeze, then sliced in 10 cm sections, melted, and the salinities determined with a conductivity meter. Parts of each 10 cm section were saved separately for subsequent analysis for quantity and origin of dirt content. Collaboration with FS POLARSTERN Helicopter The intention of this joint work was to have the Polarstern helicopters fly over all the tracks in fast ice carried out by Autosub before August 25; then for the helicopters to fly a local pattern of tracks over the 2 x 2 km experimental survey area of August 25. The towed EM bird system would provide thickness validation for the Autosub sonar. Unfortunately on the day of our meeting fog prevailed all day, and only one local flight was accomplished which had to be aborted because of failure of the laser to lock on. At this time it is not known whether any useful data were obtained. EM31 ground system The Polarstern sea ice team carried out several 500 m – 1 km transects of the experimental survey area using a manually-towed kayak carrying an EM31 electromagnetic sounding system and snow probe. Together these give snow depth and total ice thickness at high horizontal resolution (approximately ice thickness, i.e. 1-2 m). The transects included those already drilled, to provide further cross-validation. In addition, a resistivity survey was carried out of a pressure ridge to give a high-resolution view of its block structure.
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SATELLITE DATA Nick Hughes (SAMS) Timely provision of satellite data on sea ice conditions in the Fram Strait and Belgica Bank area was essential for planning fieldwork operations as the JCR lacks helicopters to carry out ice reconnaissance. There were two main sources of satellite data for JR106 Autosub-UnderIce fieldwork. AMSR, QuickSCAT and Envisat GMM data were provided by Leif Toudal of the Danish Centre for Remote Sensing and e- mailed daily to the ship by Dave Meldrum at SAMS. Acquisition of Envisat WS data to cover the fieldwork was ordered by SAMS from ESA prior to the cruise. Delivery of 4 of the scenes in near-real time (NRT) to cover 8, 17, 20 and 24 August was ordered from Kongsberg Satellite Station (KSAT) in Tromsø, Norway. Processing of the data to derive quick look images and e- mailing of these to the JCR was carried out by Richard Hall of the Norwegian Polar Institute (NPI). QuickSCAT The algorithm for the QuickSCAT sensor on the SeaWinds satellite is designed to detect the presence of low concentrations of sea ice and areas of open water. During JR106 the daily images were used to estimate the position of the ice edge and any useful areas of open water. On approaching the Belgica Bank small scattered floes were found which were well outside the area delineated as ice by the QuickSCAT. Therefore it was assumed that the algorithm was underdetecting ice and that open water areas within ice were suspect. The images are often affected by areas of high wind speed causing greater water surface roughness and appearing as ice. QuickSCAT is also a fairly low resolution (25 km) instrument and cannot resolve areas of detail. An example image from 23 August is shown to the right. AMSR 89GHz Ice The 89 GHz vertical and horizontal polarity channels of the Advanced Microwave Scanning Radiometer (AMSR) sensors on NASA’s EOS Aqua and Terra satellite are used to derive high resolution (6.25 km) maps of sea ice concentration. The high frequency makes the 89 GHz susceptible to interference from atmospheric moisture (as shown in the example from 24 August on the right). However they are good for showing areas of concentrated sea ice and some indication of lower concentrations of floes. In this image the fast ice fringing the east of Greenland is clearly shown along with a few broken-off ex-fast ice floes in Fram Strait. A weather system is visible in the eastern half of Fram Strait. NERC Grant NER/T/S/2000/00985
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AMSR Ice Concentration Lower frequency channels provided by AMSR provide good measurements of sea ice concentration (percentage cover of sea ice within an area) during autumn, winter and spring. During summer AMSR, like the other passive microwave SSM/I sensors and its predecessors SMMR and ESMR, is affected by surface melt pools. These areas of water ponded on a floe are seen by the satellite to be open water even though there is ice underneath. Therefore summer ice concentration estimates tend to be less reliable and lower than those from optical sensors. In the example above the QuickSCAT ice limit is shown as a red line and is seen to be well outside the ice limit shown by AMSR. Envisat GMM The Global Monitoring Mode (GMM) of ESA’s Envisat Advanced Synthetic Aperture Radar (ASAR) sensor is used for wide area coverage when the sensor is not tasked with specific data acquisitions. SAR or active microwave produces a high resolution image of the surface radar energy backscatter beneath the sensor. In GMM image resolution is reduced to 1 km to reduce data processing load and allow global coverage. GMM shows up the boundaries of ice and water areas as well as some large floes. This example from 23 August shows the far northeast corner of Greenland in the lower right with the fast ice encountered by the JCR stretching away down the coast to the south. Open water with waves scattering radar energy appear on the right side of the image. Open water with little or no wave activity does not reflect radar energy so well and appears as the black areas in the image. Sea ice floes and open water appear as the various levels of grey inbetween. Envisat GMM images were received on 14, 19, 23 and 25 August and were useful in supplementing the WS images received from Envisat.
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Envisat WS Envisats Wide Swath (WS) mode provides the same width of coverage as GMM but with a greater resolution of 150 metres. It was arranged that the position of JCR at the time of the satellite overpass would be e- mailed to NPI to allow the position of the ship to be marked in the image and a full resolution of an area around the ship to be produced. 8 August: The image to the left was produced before the start of JR106 and shows an expansive fast ice edge on the east coast of Greenland. This ice has already started to break-up near the far north-east tip with large floes drifting out into Fram Strait. Also visible is a distinct variation in radar energy backscatter from the fast ice closer in to the coast with that on the outer edge. It is hypothesized that this may be a division between first year and multi year fast ice and is something that a run by Autosub underneath the ice may by able to clarify. 17 August: By this date JCR was just outside the area of acquisition, the full quick look of which is shown below. However shortly after entering it on the following day a large tabular iceberg was encountered at the position shown in the full resolution image to the right. A photograph of the iceberg is shown on the following page. It is possible that some of the bright speckle seen in the SAR images are icebergs. This will be the subject of further investigation after the cruise. The large ex- fast ice floes seen 8 days earlier furthest east in Fram Strait have broken up.
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Large tabular iceberg encountered on 18 August.
20 August: On this day JCR was at the first of the ice stations on the fast ice edge. The Envisat image provided suffered from geo-correction problems in one of the bands used to produce the average backscatter values covering where JCR was located. This resulted in a double image but an extraction of a full resolution portion, shown below, clearly shows the fast ice to the north developing an east-west fissure. The fast ice further out in Fram Strait continued to drift south-east and break-up.
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JR106 Cruise Report (v1.00) 24 August: The final Envisat image, shown to the left, delivered for this portion of JR106 still shows the distinct fast ice edge between 79ºN and 79º40’N still as it was at the beginning of the series of images. The fast ice floes broken off to the north were broken up and swept down to the south by a day of storm conditions in the Greenland Sea. On the afternoon of 24 August JCR negotiated several of these bands sailing south to meet up with the German icebreaker Polarstern at the fast- ice edge. The full resolution image based
on JCR’s position at the time of acquisition is shown above. A second full resolution image shows the swirls of broken-up fast ice travelling southward along the fast ice edge. This is shown to the right. Conditions beyond this area of broken up ice were fairly open with plenty of open water for navigation exiting east from the Belgica Bank area.
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SEA ICE WATCH Steve Ackley (USA), Kieran Rutherford (SOC), Ken Collins (SOC) and Gwyn Griffiths (SOC) Introduction We conducted hourly sea ice observations while the JCR was underway from the first encounter with pack ice at 1820 on 16 August 2004, until we left the ice at 0800 on 27 August 2004. Observations were conducted according to the ASPeCt protocols developed for Antarctic sea ice (A. Worby, CD titled ‘Observing Antarctic Sea Ice’). Using the World Meteorological Organization (WMO) classification for snow and sea ice, codes are entered for each hour of underway travel, for a 1 km diameter observing area at the time of observation, describing the ice and snow. The parameters described are: total concentration, open water (distance between floes), and for up to three ice types the concentration by type, the type of ice, ice thickness, floe size, topography(area and height of ridged ice), snow type and snow thickness. The codes are entered into a sea ice log and using software available on the CD, summaries of ice conditions can be computed according to the parameters described, for example the ice and snow thickness distributions, either total or any average of track length desired. Figure 1 shows a cruise track plot with blue dots keyed according to ice concentration for example, and positions of Autosub launches and recoveries and furthest excursion shown in red. Describing sea ice in this manner therefore gives a survey of observed conditions that are comparable to other methods of data collection for sea ice, from the broad scale available from satellite data, through higher resolution and intermediate distance scales such as from Autosub upward looking swath imagery and submarine and mooring upward looking sonar from the region, and high resolution, short distance records such as the hole drilling campaigns for ice thickness conducted at the fast ice during the cruise. The accompanying data CD has two other folders along with the sea ice log. The first is of the photographs taken from the bridge (starboard, forward and port) during the ice observation when visibility conditions allowed. These are indexed to time and date and can therefore be cross indexed with the date and time of the corresponding entry in the ice log. A second folder, of satellite data images from EnviSat, are also archived. These are of the whole area on a given day and can be co- located with the corresponding log date for the short track on any given image.
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Figure 1: Ice concentrations from ship observations along Leg 1 (blue) and Autosub launch/recovery and furthest excursion positions (red).
Ice Concentration Figure 1 shows that generally low ice concentrations were observed except near the coast of Greenland where we encountered either fast ice (attached to the shore) or vast floes (>2 km diameter) that were recently broken out from the fast ice. Offshore no more than 3/10 ice concentration was observed in the pack on the inbound track while up to 5/10 was seen occasionally on the out ward bound track. The outer pack was highly dispersed, reflected in the floe sizes also, which were less than the 100 m diameter category in the outer parts indicating they were broken apart by heavy waves and swell at one time. No high concentration feature identifiable as a distinct ice edge was observed, only a broad area of dispersed floes, (Figure 2.) indicating northerly to north-westerly winds had prevailed for a length of time prior to our arrival.
Figure 2: Ice watch photo 17 August, 0100, showing dispersed floes and lack of distinct ice edge.
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Ice Types The ice types varied also with predominantly multiyear ice seen in the outer regions with thicknesses (of level ice) estimated at 200 cm. Floes with high densities of ridges were also seen occasionally which would serve to raise the mean thickness. Another indicator of the multiyear age is the observations of sediment on the surfaces of the older ice floes seen quite commonly in the outer reaches of the ice pack. Sediment in the ice originates from incorporation during first ice formation in turbulent conditions found primarily in shallow water on the Siberian Shelves such as in the Laptev and Kara Seas. The sediment accumulates progressively on the surface as ice melts during summer, so darker floes have drifted long enough to last through two summers’ melt.
Figure 3. Sediment on surface of floe (dark area) in photo center also some lighter, smudgy areas of sediment on floe i n the foreground, 19 August 0300.
At the fast ice, proportionally larger amounts of first year ice were seen, with thicknesses in the 1 to 1.5m categories and only very occasional bits of thicker ice with sediment showing. Ridging was also quite low in the first- year ice seen in the fast ice, reflective of the growth in quieter conditions and younger age as it attached or nearly attached to the shore at the time of its formation. From the 21 to 26 August, we observed new ice formation conditions (grease ice and nilas, to 10 cm thickness). On the last days, 25 and 26 August, these new ice types survived past midday suggesting the end of the summer season and beginning of the ice growth period was initiated at this time. Surface Conditions (Snow Cover and Melt Ponds) In the early part of the cruise, the full melting condition of the summer pack was in evidence. Estimates of melt pond coverage (tested at low salinity as essentially fresh water from snowmelt) were generally from 15 to 25% coverage of the ice surface. In almost all cases, however, there was approximately a 10 cm thick snow cover remaining throughout the region between the melt ponds (Figures 3 and 4). Some melt ponds were observed to completely perforate the floe to the ocean below. The sno w cover was highly metamorphosed, with ~0.5 cm grains indicative of the grain growth that takes place when the snow is saturated with melt water. Channels into and between melt ponds also were evident showing the pathways of water flow from the higher topography of the floe to the low spots where the water pooled. (Figures 3 and 4).
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Figure 4: 18 th August 1700 showing melt ponds and channels at full development of summer melt. Snow cover is still present but fully ‘ripened’ with large grains.
From the 22 August, new snow accumulated on the floes, measured at 5 to 10 cm from the surface measurements. Melt ponds were also frozen over with a thin layer of new ice starting from this time (Figure 5), another indicator of the transition to fall- winter conditio ns and the start of the ice growth season, as indicated by the new ice types observed as noted above.
Figure 5: Photo from 26 August, 1500 showing frozen-over melt ponds and new snow cover at start of fall-winter transition in NE Greenland.
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PHYSICAL OCEANOGRAPHY Jeremy Wilkinson (SAMS) and Terry Edwards (UKORS) The main aim of the physical oceanography programme was to support the Autosub operation in and around the North East Water Polynya. As a result physical oceanographic measurements were obtained from the ship-borne Seabird 911, the AUV mounted Seabird 911 system and a hand held SBE 19. All systems are described below: Ship borne unit: The on-board CTD unit was the Sea-Bird 9 plus (Ser: 0528) with duel temperature and conductivity sensors, SBE 43 oxygen sensor, Chelsea instruments MkIII fluorometer, Chelsea Instruments Alphatracka 25cm 660nm Transmissometer, Benthos PSA/916T Altimeter and a Digiquartz Pressure transducer. The temperature, conductivity and oxygen sensors were attached their respective pumps. The above instruments were attached to the bottom of the SBE32 carousel (Ser: 0344) (see picture left). There was the possibility to mount up to 24 bottles on the carousel, however our set up required only 8 bottles to be attached. There was also a RDI LADCP 300 kHz system attached to the upper and lower brackets of the carousel. The distance of separation between the 2 ADCP units was approx. 106 cm + each sensor was approximately 24 cm tall. The date of the last calibration and serial numbers for the oceanographic sensors can be seen in Table 1. A full copy of the calibration coefficients for all instruments can be obtained from the PSO. Channel
CTD Serial Date of calibration Sensor Number 1. Frequency Temperature 4116 9/6/04 2. Frequency Conductivity 2407 17/6/04 3. Frequency Pressure, Digiquartz 73299 8/5/02 with TC 4. Frequency Temperature 2 2919 9/6/04 5. Frequency Conductivity 2 2450 17/6/04 6. A/D voltage 0 Oxygen, SBE 43 0619 16/6/04 7. A/D voltage 1 Free Free Free 8. A/D voltage 2 Altimeter 874 23/4/01 9. A/D voltage 3 Fluorometer, Chelsea 88195 27/3/03 Aqua 3 10. A/D voltage 4 Free Free Free 11. A/D voltage 5 Free Free Free 12. A/D voltage 6 Optical BackScatter, N/A N/A Seatech LS6000 13. A/D voltage 7 Transmissometer, 161045 28/4/01 Chelsea Aphatracka 25cm 660nm Table 1: CTD configuration used throughout JR106 for ship-borne CTD
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Once we arrived at the designated station the CTD was ‘made ready’ by either Terry Edwards (12 pm to 12 am) or Pat Cooper (12 am to 12 pm). The deployment of the CTD was from the starboard mid-ship’s gantry via an A frame. The logging was generally initiated using SeaSave the Seabird data acquisition software before the CTD was in the water. The salinity and temperature values were monitored until they were stable and then the CTD was lowered at about 1m/s. Water samples were ‘fired’ on the up cast in water identified by the down cast as having a low T and S gradient. At the end of a station the CTD was taken back on deck and fastened to the ship before heading to the next station. The procedure of keeping the CTD outside should be avoided as we have had experiences on other cruises of the conductivity cell freezing and breaking in below freezing temperatures. This has occurred in instances of when the CTD has been outside for only a few minutes. Autosub unit: The instrument on board Autosub is a standard SBE9 plus. This pumped system had an inlet manifold at the front of the AUV. The system ran duel temperature and conductivity sensors, SBE 43 oxygen sensor and a Digiquartz Pressure transducer. The date of the last calibration and serial numbers for the oceano graphic sensors can be seen in Table 2. A full copy of the calibration coefficients for all instruments can be obtained from the PSO. Channel
CTD Serial Date of calibration Sensor Number 1. Frequency Temperature 2342 25/07/03 2. Frequency Conductivity 2730 18/03/04 3. Frequency Pressure, Digiquartz 89080 2/26/02 with TC 4. Frequency Temperature 2 2912 6/21/02 5. Frequency Conductivity 2 2760 7/10/02 6. A/D voltage 0 Oxygen, SBE 43 0259 01-May-02 7. A/D voltage 1 Free Free Free 8. A/D voltage 2 Free Free Free 9. A/D voltage 3 Free Free Free 10. A/D voltage 4 Free Free Free 11. A/D voltage 5 Free Free Free 12. A/D voltage 6 Free Free Free 13. A/D voltage 7 Free Free Free Table 2: CTD configuration used throughout JR106 for Autosub CTD
From Table 2 it can be seen that in general the date of calibration for most of the instruments is quite old. These instruments will be calibrated on return to the UK. The set up and logging of the instrument was controlled by the Autosub team. Hand-held CTD: In order to obtain the temperature and salinity profiles of the upper 50 m away from the influence of the ship a hand held SBE 19 was used. This system has been used successfully in the past both from a zodiac and from an ice floe. However due to the work-load it was not possible to use this CTD in anger except on one occasion from the side of the ship. The one deployment was designed to monitor the upper 1 –2 m of the sea ice melt layer. To do this the system, which was connected to a buoy
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by a rope 1.5m long, was lowered over the side of the JCR. The pumped SBE-19 was recorded the T and S of the upper 1.5m every 0.5secs. The system was designed to free float away from the ship. The same rope that was used to lower the instrument was used to bring it on board. CTD Post processing: As the manufacturer, Sea-bird, was common to all three CTD systems the SBE Data processing software (5.1.26) was used to process and convert the data into ASCII. However the exact scripts used varied depending on the instruments. To run the data processing sequences an up to date configuration (.con) file for each instrument was needed. The data processing sequence used on this cruise is as follows: datcnv alignctd filter celltm loopedit derive
(this was not run on the AUV based system)
To make life easy the above data processing scripts were included in a batch file, which was run in windows. An example of the batch file to process the ship based CTD was as follows: @ Lines starting with @ are comment lines @ Select Run in the Windows Start menu and run this line: @ sbebatch D:\jeremy\jcr106\ctd\seabird911\prallcasts_jcr.txt D:\jeremy\jcr106\ctd\seabird911 @ Comment lines have no effect on the results datcnv /i%1\*.dat /c%1\CTD_001.con /o%1 alignctd /i%1\*.cnv /o%1 filter /i%1\*.cnv /o%1 celltm /i%1\*.cnv /o%1 loopedit /i%1\*.cnv /o%1 derive /i%1\*.cnv /c%1\CTD_001.con /o%1
Each line in the batch file runs a different SBE Data Processing module. These modules are explained below and are generally taken directly from the Seabird manual. Data Conversion (datcnv): This programme converts raw data (.dat file) into ASCII file (.cnv format) as well as bottle data. As we planned to post-process the data with other SBE Data Processing modules, we selected only the primary variables to be converted. These were: For ship mounted system: # # # # # # # # # #
name name name name name name name name name name
0 1 2 3 4 5 6 7 8 9
= = = = = = = = = =
prDM: Pressure, Digiquartz [db] c0mS/cm: Conductivity [mS/cm] t068C: Temperature [ITS-68, deg C] c1mS/cm: Conductivity, 2 [mS/cm] t168C: Temperature, 2 [ITS-68, deg C] sbeox0Mg/L: Oxygen, SBE 43 [mg/l] flC: Fluorescence, Chelsea Aqua 3 Chl Con [ug/l] xmiss: Beam Transmission, Chelsea/Seatech/Wetlab CStar [%] altM: Altimeter [m] v6: Voltage 6 (BOB)
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For the AUV system: # # # # # # # #
name name name name name name name name
0 1 2 3 4 5 6 7
= = = = = = = =
prDM: Pressure, Digiquartz [db] c0mS/cm: Conductivity [mS/cm] t068C: Temperature [ITS-68, deg C] c1mS/cm: Conductivity, 2 [mS/cm] t168C: Temperature, 2 [ITS-68, deg C] sbeox0Mg/L: Oxygen, SBE 43 [mg/l] timeS: Time, Elapsed [seconds] timeJ: Julian Days
Align CTD (alignctd): Align CTD script aligns parameter data in time, relative to pressure. This ensures that calculations of salinity, dissolved oxygen concentration, and other parameters are made using measurements from the same parcel of water. When measurements are properly aligned, salinity spiking (and density) errors are minimised, and oxygen data corresponds to the proper pressure. For the SBE 9plus the typical lag of conductivity relative to temperature is 0.073 seconds. The Oxygen data is also systematically delayed with respect to pressure. The two primary causes are the long time constant of the oxygen sensor, approximately 5 seconds at out sea temperature and an additional delay from the transit time of water in the pumped plumbing line. We compensated for this delay by shifting oxygen data relative to pressure 5 seconds. No shifts to conductivity were performed. Filter (filter): Filter runs a low-pass filter on one or more columns of data. A low-pass filter smoothes high frequency (rapidly changing) data. To produce zero phase (no time shift), the filter is first run forward through the data and then run backwards through the data. This removes any delays caused by the filter. Only conductivity and pressure data were filtered but at different time constants. These were: Low pass filter A: 0.03 seconds for conductivity Low pas filter B :0.15 seconds for pressure. Loop Edit (loopedit): Loop Edit marks scans bad by setting the flag value associated with the scan to badflag in input .cnv files that have pressure slowdowns or reversals (generally caused by ship heave). The badflag value is documented in the input .cnv header. Loop Edit operates on three successive scans to determine velocity. This is such a fine scale that noise in the pressure channel from counting jitter or other unknown sources can cause Loop Edit to mark scans with the badflag in error. As a result Loop Edit must be run after Filter on the pressure data to reduce noise in the pressure data. Sea-Bird recommends using a pressure time constant in Filter equal to approximately the time required for four scans. Thus for the SBE9 plus sampling at 24 Hz, we used a time constant of 0.125 seconds (time required for 4 scans). Due to the possible porpois ing of the Autosub this procedure was not run on the AUV data. Cell Thermal Mass (celltm): Cell Thermal Mass uses a recursive filter to remove conductivity cell thermal mass effects from the measured conductivity. In areas with steep temperature gradients, the thermal mass correction is on the order of 0.005 PSU. In other areas the correction is negligible. Values for alpha and 1/beta were 0.03 and 7.0 respectively for both the primary and secondary temperature sensors.
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Derive (derive): As we post-processed the data with other SBE Data Processing modules we selected only the primary variables to be converted up to this stage. We now used Derive to compute derived oceanographic parameters; Salinity and Oxyge n. Derivation of other variables, e.g. salinity, density, potential temperature etc were performed in Matlab according to the Unesco technical papers. Temperature IPTS-68 were used in these computations. According to JPOTS t68 is assumed to be 1.00024 * T90 (-2 to 35C). Calibration of the CTD data CTD Performance 20 CTD profiles were carried out, most shallow, one to 2500m. 4 samples were taken from each profile for salinity checks. NMEA lat and long were added to the header file as was time synchronised to the ships clock. GGA was used as RMC string was not available. Temperature and conductivity pairs performed well, however an offset appeared of .003 PSU between primary and secondary salinities on cast 20, showing up when in the stable section of the water column. This will be compared with salinity samples. Pressure sensor performed well. On a number of casts there were a small amount of spikes in the data, though the cause of these could not be determined as the problem was very sporadic and not repeatable. The rogue data was removed during processing. Oxygen sensor did not perform well exhibiting varying amounts of hysterisis on most casts. On cast 20 (2500m) the downcast appeared normal. The upcast showed no profile at all, the oxygen signal tapering off towards 2mg/l. This problem to be investigated. The entire ductings had been cleaned with milli Q water after every cast, but stored empty in case of freezing. Carousel performed without problems. Altimeter performed well, the usual spikes until it locked on, usually at around 70m from bottom. LSS , transmissometer and fluorometer all performed without problems. Salinometry Refer to the accompanying spread sheet. It is shown that through out the series there has been a large variability between measured sample and CTD reading. This is due to the nature of the water column and associated instability. This is demonstrated clearly on cast 20 where the samples correlate very well, they were taken in deep water. The offset between primary and secondary salinities shown on cast 20 is likely due to a build up of biological growth in the conductivity cells. Samples 0-12 were performed on the BAS salinometer s/n 65763. However, due to problems with air bubbles in the system all other sampling was carried out on OED salinometer 56747. All samples in the file marked 9999 are std seawater run to check standardisation. NERC Grant NER/T/S/2000/00985
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The salinometer was finally restandardised prior to running crate 11. First results Ship based: A total 20 full depth CTD stations were performed on JR106. The term ‘full depth’ is a bit misleading as most of the casts were in shallow water less than 200 m. The time of the casts and their location with respect to bathymetry and topography can be seen below: Station
Time
Latitude
Longitude
Depth
1 2
18/8/04 10:48 PM 19/8/04 6:43 AM
78.8454 79.2891
-6.4166 -8.5097
298 172
3 4 5
19/8/04 5:45 PM 19/8/04 8:38 PM 20/8/04 4:04 AM
79.3703 79.3982 79.4945
-9.8712 -9.9315 -11.8022
172 180 214
6 7 8
20/8/04 7:40 AM 22/8/04 11:16 AM 22/8/04 1:26 PM
79.5046 79.5052 79.4985
-14.1134 -14.2141 -14.2538
105 131 105
9 10 11
22/8/04 2:24 PM 23/8/04 5:16 PM 23/8/04 6:14 PM
79.7395 80.2705 80.3447
-14.2115 -13.0817 -13.3130
87 165 282
12 13 14
23/8/04 7:26 PM 23/8/04 9:07 PM 24/8/04 1:26 AM
80.4171 80.4801 80.3583
-13.5613 -13.9038 -12.7806
281 317 256
15 16 17
24/8/04 6:28 AM 24/8/04 7:55 AM 24/8/04 9:21 AM
80.4299 80.5056 80.4927
-12.5313 -12.7839 -12.1823
290 295 280
18 19 20
24/8/04 10:33 AM 24/8/04 11:45 AM 27/8/04 10:04 AM
80.5735 80.6448 77.6053
-12.0443 -11.7938 -4.1118
270 264 2556
After batch processing was performed on the CTD data the resultant CNV file was then imported into Matlab for analysis. This proved very handy as we could produce plots and sections instantly. At this stage no other processing was performed to the data. An example of the hydrography over the Belgica Bank can be seen below. In this figure one can see a shallow fresh sea ice melt layer in the upper surface, under which lies water of Polar origin and finally under this layer is Atlantic based water.
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Potential Temperature
Salinity
Potential Density
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First results Autosub: The processing of CTD data from the Autosub was slightly more complex than the ship-borne system as positional information had to be married to the .CNV file before it became usable. This occurred by running a series of matlab scripts that were written by JW whilst on board. These were in order of processing: 1. The first m- file loaded both the .CNV file and the navigational file .bnv from Autosub and interpolated the navigational data to the same resolution as the SBE 9 plus, i.e. 24Hz. 2. Once this was accomplished a second m- file removed all data when the Autosub was on the surface, i.e. above 5 m depth in our case. If two or more missions were run without the Autosub coming on board a different m- file would split the data into separate missions before removing data from the upper 5m. 3. The third m- file plotted each variable in turn and asked the user if it needs to be filtered (i.e. data spikes removed). If the data is particularly noisy it was filtered by calculating the mean and standard deviation over a user specified window size over the entire data. Data above a used defined number of standard deviations was removed. This procedure can be repeated a number of times. 4. The final m- file averages the data into user defined time steps. In our case data was averaged in to 1 second bins. 5. The final m- file plotted the data. An example of the output from this file can be seen below.
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MARINE TECHNOLOGY TESTS Duncan Mercer (SAMS) Greenland Arctic Shelf Ice Experiment (GreenIce)
Green Ice “buoy” on a previous deployment.
As part of the international Greenland Arctic Shelf Ice Experiment (GreenIce) project, an ice thickness measuring “buoy” was deployed onto a area of thick ice near to the ship. The buoy’s position was chosen such that it was close to the centre of an area that had been surveyed previously, both by drilling and by an autosub swath mission. This location was chosen in order to allow cross comparison of various measurement methods. In addition to the measurements made by the JR106 team a series of E.M. measurements were made of the same area by the German teams from Polarstern.
This buoy was the fifth of the SAMS GreenIce buoys to be deployed (perversely enough the instrument was designated GreenIce01). The previous four buoys having been deployed north of Ellsmere Island in the Canadian Arctic ocean at latitudes of around 85ºN. These buoys that were developed at SAMS are designed to make use of work by Nagurny. This work allows area averaged ice thickness “measurements” to be derived from measurements of ice dynamics. The Nagurny method requires observations of the periods of flexural waves passing through the sea ice cover. These waves are generated by storms on the ice edge and then propagate across the Arctic Ocean through the ice cover. In the deep pack these waves have peak to peak amplitudes of around 1mm and periods of 30 seconds or so, though at the site for GreenIce01 these amplitudes were expected to be significantly larger. The primary sensor of these GreenIce buoys is a sensitive tiltmeter, this has to be able to resolve tilts in the surface ice cover, of the order of microradians. In order to provide these high resolution measurements, the buoy has an arrangement of stepper motors which provide a self levelling capability this ensures that the sensor can be correctly levelled at the start of each measurement cycle. Once deployed the buoy is not expected to be recovered and transmits it’s data across the Iridium satellite phone ne twork. GreenIce01 was deployed onto the ice at 07:00Z 26/08/2004 at a position 79º19.87’N, 013º50.70’W. By the time of the buoys first measurement cycle at 18:00Z the buoy was lying on its side, all three of the independent tilt sensors (main, gross and “topple over”) out of range. Given the carefully chosen deployment area of solid ice, and the buoy’s inherent stability (wide base and very low centre of gravity) this “falling over” is extremely suspicious. The most likely explanation is polar bear activity. A set of tracks was seen in the snow prior to deployment and four bears were sighted in the area an hour or so after leaving the floe. At the time of writing it is hoped that a ship from the Norwegian Polar Institute may be able to visit the site sometime in the following month and investigate and right the buoy.
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DWOS deep water Acoustic Modem trials The DWOS (Deep Water Observing System) project is part of the UK’s commitment to OSPAR (European Union, Oslo-Paris Accord). The aim of the project is to provide long term, real time measurements, of certain key water quality parameters. These measurements are to be made over the whole water column, off the edge of the UK continental shelf in water around 2-3 km deep. The JR106N cruise provided the ideal opportunity to test one of the key elements of the DWOS system, the acoustic telemetry link, in deep water. The acoustic modem link (along with an Iridium satellite link) will enable real time two way communications with the DWOS profiling instruments when they are ultimately deployed in the North East Atlantic. The aims of the short trial on JR106 were to test some of the manufacturers claims about the acoustic modem selected for DWOS (a LinkQuest 4000), and to provide a series of controlled operatio nal tests. These tests will ultimately be used to provide operational input into the final “Acoustic modem trial” mooring being deployed. development of the DWOS profiler. The modem uses a spread spectrum chirp frequency range (12-20 KHz) and claims to provide a robust error corrected link across tha t channel. The short mooring string (around 7m long) consisting of modem, release, anchor and buoyancy was deployed into 2500m of water at a position 77º36.33’N, 004º06.69’W. After deploying the mooring the JCR was allowed to drift such that the range from the mooring site gradually increased. This drift allowed the testing of the acoustic link between surface and seabed at a number of different distances. At each of the ranges a number of different data streams were transmitted surface to seabed and then back again, allowing some of the performance characteristics to be established. Data packet sizes of up to 10Kbytes were transferred. Initial results suggest that the link performed extremely well when the surface, seabed offset was 1000m or less. At greater ranges the performance was not quite as good as anticipated, though some of the problems might be related to the high background noise levels associated with ships. These trials suggest that the modem system will be suitable for use in the DWOS project, they do however highlight the need for the careful design of the transfer protocols to enable the system to cope with the more extreme ranges. Further consideration of the test results should inform this design of transfer protocol.
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ALONG TRACK MEASUREMENTS Jeremy Wilkinson During the cruise the along track loggers recorded a number of meteorological and oceanographic parameters. In total 12 meteorological and 3 oceanographic parameters were logged. Both the oceanographic are meteorological parameters are explained below: Oceanographic parameters Oceanographic parameters recorded by the oceanlogger system which comprised of a thermosalinograph and fluorometer both of which were connected to the ship’s non-toxic seawater supply. These parameters were recorded every 2 seconds. However due to our passage through ice covered seas the pumps to the logger were turned off in order for the sensors not to be damaged by ice. Time stamped bottles were taken to calibrate the salinity sensor. Meteorological Parameters A suite of meteorological sensors are on board JC. These include wind direction and speed, air temperature (x2), relative humidity (x2), barometric pressure (x2), Photosynthetic Active Radiation (x2), Solar Radiation (x2). Generally these instruments recorded at 2 second time intervals. Other instruments Other instruments that are generally logging continuously include the 5 navigational instruments, (Trimble 4000, Ashtec GG24, Ashtec ADU-2, Gyrocompass and Electromagnetic log) and a number of acoustic devices e.g. EM120, EA600, EK60 and TOPAS. Database The JCR database stores all along track data recorded during the cruise. This data can be accessed by a series of commands. Unfortunately we only had time to learn a few of the commands. Data processing: Due to our lack of knowledge of the onboard PSTAR software we spent the first few days writing scripts in UNIX, PERL and Matlab to process the along track data. A PERL script by Duncan Mercer merged all the meteorological, oceanographic, depth from the EM120 and positional information in to one time stamped file. This script was automatically run once a day using the crontab function. A Matlab m- file by Jeremy then processed the data. An example of the daily plots that were made available to all on board can be seen below:
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Figure: Visual display of the daily oceanographic and meteorological parameters logged on the 14 August 2004.
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EM120 MULTIBEAM SWATH BATHYMETRY AND TOPAS Jeffrey Evans (SPRI) and Colm Ó Cofaigh (SPRI) 1. Introduction EM120 12 kHz multibeam swath bathymetric and TOPAS data was acquired continuously during the transit to, and from Iceland, and in the main study area of NE Greenland and the Fram Strait. This section provides an overview of the geophysical methods and data acquired from the NE Greenland continental shelf and adjacent slope along the western side of the Fram Strait. Data acquired during the transit to, and from Iceland, are not included here. Watch-keeping of the EM120 and TOPAS workstations was carried out by Jeffrey Evans (SPRI), Colm Ó Cofaigh (SPRI), Ruth Mugford (SPRI) and Zoe Roberts (SOC). 2. Data acquisition 2.1.1 EM120 Swath Bathymetry The Kongsberg-Simrad EM120 multibeam swath bathmetry system was operated throughout the cruise. Angular coverage was set to “Manual” and beam spacing was set to “Equidistant”. The beam angle used varied according to sea conditions, water depth and seabed type but was generally between 60-68 degrees. During surveys, overlap between individual swath lines was achieved by means of the Helmsman’s Display on the bridge, which the Bridge Officer used to adjust the ship’s course and maintain a reasonable degree of overlap (10%) between lines. Limited post-processing of the EM120 data (gridding and data filtering) was carried out using the Kongsberg-Simrad NEPTUNE post-processing software. In general the EM120 worked well in water depths down to about 3000 m throughout the cruise, especially in shallow water (<1000 m) on the continental shelf. Where the system lost the sea-bed from time to time the most useful method was to use the “Force Depth” command with a depth slightly less than the true seabed. Restricting the maximum and minimum depths to a tight range around the true seabed depth was also useful. The EM120 system performed well and problems encountered during previous cruises (notably with regard to the SSU on cruise JR84) were absent. The most significant problem that we did encounter concerned the map projection used on the transit survey north. We initially selected ”UTM” from the options available in the Merlin software. However above 78 degrees north the survey became unstable and would frequently crash when using the mouse to move around on the logging workstation screen. This problem was particularly prevalent when trying to set up the “Bridge Display”. Resolution of this problem could be achieved by creating a separate map projection for the UTM zone of the survey. This is a relatively straightforward solution when engaged in the surve y of a specific area. However, during long transits it is less satisfactory as it would necessitate the progressive creation of a series of projection files. We solved this problem by check/replaying the transit lines on the NEPTUNE (processing) workstation, which then allowed us to select a different projection for the survey (Mercator 60). The survey was then exported back to the logging disk and reopened on the logging workstation with the new projection. This appeared to solve the proble m and no more crashes occurred. As on previous cruises where the EM120 was used in pack ice (JR84 and JR104), it was found that when the ship was moving through the ice the swath signal deteriorated significantly. However, the signal returns in only a few metres of open water. The EM120 acquisition parameters used are described below:
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MBES screen Ping Mode: Auto Sector Coverage Max Port Angle: 50-70 Max Starboard Angle: 50-70 Angular Coverage: Manual Beam Spacing: Equidistant Pitch stabilisation: On Yaw stabilisation: Off Min depth: Used to constrain depth when bottom is lost Max. depth: Used to constrain depth when bottom is lost Sound Speed Profile Current Sound Profile: jr104_xbt??.asvp Sound Speed at Transducer: From: Profile Sensor Offset: 0.0 m/s Filter: 60s Filtering Spike Filter Strength: Aeration: Sector Tracking: Slope: Interference: Range Gate: Absorption Coefficient Absorption (dB/km): Seabed Imaging TVG Crossover (deg)
Medium Off On On Off Normal 1.00 6
2.1.2 TOPAS Sub-Bottom Profiler and EPC Chart recorder The TOPAS system was used extensively throughout the cruise and generally performed very well. As in the case of the EM120, sea ice affects the TOPAS signal quite badly. It results in many high amplitude signals resulting in dark traces across the record. In heavy sea ice this can have the result of obliterating any meaningful data. In water depths of less than 1000 m we ran TOPAS using a Burst mode whereas in depths greater than this we used the Chirp. TOPAS acquisition parameters are outlined at the end of this section. The EPC chart recorder worked without any problems throughout the cruise. TOPAS input to the EPC chart recorder was on Channel A. The settings used were: 0.5 second sweep; 0 delay; threshold 1/3 of a turn clockwise from the minimum setting; trigger level 0; gain generally about 8-10; sweep direction from left to right; print polarity +/- (centre setting). Chart settings: scale lines: on; take-up: on; mark/annotate: off (centre setting); chart drive: internal (centre setting), LPI was generally set to 75; contrast setting: centre. Ten- minute time and EM120 centre depth data were relayed to the 9800 Series Graphic Recorder Computer and were automatically marked on the EPC Chart Recorder paper roll. On occasions the time and EM120 centre depths were not marked on the paper roll. This required a system reboot of the 9800 Series Graphic Recorder. This is carried out NERC Grant NER/T/S/2000/00985
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by: (a) ALT-X to Exit the software; (b) selecting ‘Return to DOS’ from the menu; (c) System reboot (flick main computer button off and then on); (d) Let system boot up and then select ‘Acquisition mode’ and the plotter will begin to automatically send time and EM120 centre depth data to the EPC paper roll. (a) TOPAS Acquisition Parameters in <1000 m water depth Parasource Menu Level: Ping Interval: Pulseform: Period: Secondary Frequency:
100% 0 ms (enables external SSU triggering) Burst 1 or 2 2800 Hz
Acquisition Menu Ch_no: Speed of Sound (m/s): Sample Rate: Trace Length (ms): Gain: Filter: Delay:
0 1500 20000 Hz 400 12 – 28 dB 1.00 kHz Manual
Processing Menu Channel no: Filter:
Processing (deconvolution): Swell:
TVG:
Deverb: Stacking: AVC: Scale (%):
0 ON Low stop: 1200 Low pass: High pass: 1700 High stop: OFF ON Threshold: 60% # traces: 1 OFF or AUTO or Man (all used at different times) Slope: (30 – 60 dB slope) Start point: Manual or Tracking or External
4800 5200
OFF
LOG/Replay Menu Medium: Rate (ms): Channel: File size (Mb):
OFF OFF 700 – 1000
Attribute:
INST.AMP
DISK 1000 0 10
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(b) TOPAS Acquisition Parameters in >1000 m water depth Parasource Menu Level: Ping Interval: SSU triggering) Pulseform:
90 – 100% 2000 – 5000 ms (Manual triggering over rides
Period: Secondary Frequency:
Chirp Chirp start frequency (Hz): Chirp stop frequency (Hz): Length (ms): 1 or 2 2800 Hz
Acquisition Menu Ch_no: Speed of Sound (m/s): Sample Rate: Trace Length (ms): Gain: Filter: Delay:
0 1500 20000 Hz 400 20 – 32 dB 1.00 kHz Manual or External
Processing Menu Channel no: Filter:
Processing (deconvolution): Swell:
TVG:
Deverb: Stacking: AVC: Scale (%): Attribute:
1500 5000 15
0 ON Low stop: 1200 Low pass: High pass: 1700 High stop: DECONV Filter factor (ppm): 1 ON Threshold: 60% # traces: 1 OFF or AUTO or Man (all used at different times) Slope: (30 – 60 dB slope) Start point: Manual or Tracking or External
4800 5200
OFF
LOG/Replay Menu Medium: Rate (ms): Channel: File size (Mb):
OFF OFF 1000 – 3000 INST.AMP
DISK 1000 0 10
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2.1.3 SSU – Sonar Sequencing Unit The SSU was used throughout the cruise to synchronise the EM120, EA600 and TOPAS systems. The bridge echosounder (EA600) was run on passive, external trigger, and listened out for the EM120 centre-beam return and used this to calculate depth below the ship. Whenever, the EM120 was not active the EA600 was switched to Active, internal triggering. The TOPAS was triggered by the SSU in water depths shallower than 1000 m. In water depths deeper than 1000 m the TOPAS was internally triggered at 2000 – 5000 ms ping intervals. The main settings used on the SSU are listed below: Group:
EM & EA, EK, TOPAS
Trigger:
EM120 & EA600: ON (both systems) EK60: OFF TOPAS: ON EM120 & EA600: Calculated (both systems) EK60: OFF TOPAS: Calculated Not used for any of the systems
Time usage:
Time add on:
2.1.4 Expendable Bathythermograph (XBT) System Eight XBT casts were made during JR106 (North) (see Table 1). Five were deepwater T5 probes that record to 1830 m water depth. The remaining three were shallow water T7 probes that record to water depths of 760 m. All the XBT deployments were successful and the sound velocity profiles (SVP) input to the EM120 and used in the relevant surveys. Only a small number of XBT’s were required during the cruise as the SVP remained fairly consistent within the study area. The SVP’s used on the northbound transit were also used southbound. The XBT system on the James Clark Ross worked well throughout the cruise. Individual SVP profiles were calculated from the XBT data by the system software, assuming a constant salinity. Salinity values were obtained from the Oceanlogger display (located in the UIC), and input to the XBT system software manually. The seawater supply to the Oceanlogger was switched off for periods during our work on the continental shelf due to problems caused by sea ice. On these occasions the most recent valid salinity measurement was utilised. The *.edf files (calculated sound velocity profiles) generated by the XBT system software were transferred to the multibeam data processing workstation, and the data then imported into the multibeam data acquisition system across the network. Table 1. Summary of XBT stations. Cast T7 - 1 T5 - 2 T5 - 3 T5 - 4 T5 - 5 T5 - 6 T7 - 7 T7 - 8
Filename T7_00011 T5_00012 T5_00013 T5_00015 T5_00017 T5_00019 T7_00021 T7_00023
Time/date 15:31:55 08/14/2004 11:38:15 08/15/2004 20:23:03 08/15/2004 19:07:06 08/16/2004 11:26:37 08/18/2004 17:14:37 08/18/2004 22:10:15 08/21/2004 19:50:03 08/23/2004
JDay 227 228 228 229 231 231 234 236
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Latitude N Longitude W 67° 32.146’ 22° 48.999’ 70° 37.036’ 15° 40.105’ 71° 55.365’ 12° 17.006’ 76° 15.666’ 7° 0.285’ 78° 38.338’ 0° 28.6289’ 78° 49.744’ 4° 13.652’ 79° 29.525’ 14° 11.447’ 80° 21.902’ 13° 23.053’
Geographical location Northern Iceland continental shelf Scoresby Sund continental slope Greenland sea NW of Jan Mayen NE Greenland continental slope Fram Strait Fram Strait Northwind Shoal, NE Greenland Shelf trough north of AWI Bank
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2.1.5 Oceanlogger The Oceanlogger was operated during JR106 (North) in order to monitor changes in surface water characteristics that affect sound propagation, and to measure surface water salinity values for calculation of SVP’s from XBT data. The Oceanlogger did not operate during our work in the ice on the continental shelf as the pump supplying seawater to the logger had to be stopped as fragments of ice clogged the filters. The seawater pump was operational during the north and south transits and also across the continental slope and parts of the shelf of the study area.
Figure 1. Unprocessed EM120 swath bathymetry acquired along the JR106 (North) track lines across the NE Greenland continental shelf. The Belgica Bank, Northwind Shoal and AWI Bank are marked.
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2.2 Results and preliminary interpretations 2.2.1 Bathymetry The NE Greenland continental shelf in the study area comprises a prominent shallow bank complex that is sub-divided into three main regions, the Belgica Bank in the south and west, Northwind Shoal to the west and the AWI Bank to the north. Water depths across these banks are 70-140 m (Fig.1). The bank complex is incised by a NW-SE trending trough with water depths of 145-300 m that extends to the outer shelf (Fig.1). A prominent W-E trending bathymetric trough also extends from the inner to the outer shelf north of the AWI Bank. Water depths in this trough range are 230-330 m and progressively deepen towards the inner shelf to the west, and north (Fig.1).
Figure 2. Unprocessed EM120 swath bathymetric shaded relief image of subglacial lineations in the cross-shelf bathymetric trough to the north of AWI Bank. The bedforms record former ice sheet flow to the east. Grid cell size = 30 m x 30 m.
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2.2.2 Subglacial bedforms and iceberg scours Streamlined subglacial bedforms and iceberg scours are observed on the swath bathymetric and TOPAS records from the NE Greenland continental shelf (Figs. 2 & 3). The subglacial bedforms provide evidence for an extensive Greenland Ice Sheet that extended onto the outer continental shelf of NE Greenland, and probably reached the shelf edge. Subglacial lineations (>5.7 km in length and <0.4 km in width) are widely distributed and well preserved in the W-E trending bathymetric cross-shelf trough north of AWI Bank (Fig. 2). The distribution of bedforms within the trough indicate that the Greenland Ice Sheet drained eastwards following the convergence of flow emanating from Dijmphna Sund and Ingolf Fjord region of NE Greenland. The highly attenuated form of the lineations suggests that this outlet may have been fast flowing. Subtle subglacial lineations (>4.3 km in length and <3.5 km in width) and ice-moulded bedrock are present within the NW-SE trending trough running between Belgica Bank, Northwind Shoal and AWI Bank indicating that palaeo- ice flow was channelled to the southeast across this area of the shelf. Subtle streamlined bedforms also occur on Northwind Shoal indicating ice flow to the northeast across this shallow shelf (Fig. 3). TOPAS records indicate that the subglacial bedforms are formed in the surface of an acoustically transparent sediment layer that has a distinct continuous sub-sea floor basal reflector. This layer is interpreted as a till unit. TOPAS records from the trough east of Northward Shoal i.e. east of 14°30’W, are dominated by a series of reflectors that dip towards the shelf edge. This unit is interpreted as a ‘till delta’ or grounding- zone wedge where subglacial sediment was advected to the ice-sheet margin. These sediments are overlain and truncated by the acoustically transparent sediment unit in which the streamlined subglacial bedforms occur. This implies that the ice advance, which formed the bedforms, occurred after the formation of the grounding- zone wedges and, therefore, that these ice- marginal features are probably a result of deposition during ice-sheet advance rather than retreat.
Figure 3. Unprocessed EM120 swath bathymetric shaded relief image of iceberg scours and subtle subglacial bedforms across Northwind Shoal on the NE Greenland continental shelf. Bedforms indicate that former ice sheet flow is to the NE. Grid cell size = 30 m x 30 m.
Swath bathymetric and TOPAS records indicate that the Belgica Bank, Northwind Shoal and AWI Bank for the most part, are dominated by discrete iceberg scours that are irregular to linear in form (Fig. 3). Iceberg scours are either randomly orientated or they have a preferred N-S, NW-SE or NE-SW orientation (Fig. 3) suggesting a strong influence of the southward flowing East Greenland Current on iceberg trajectories. TOPAS records indicate that iceberg scouring of the sea floor has homogenised the sedimentary record in this region.
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TOPAS records from the continental slope adjacent to this region of the NE Greenland continental shelf comprise widespread, stacked, acoustically- transparent sediment bodies. These bodies are lens-shaped in an along-slope direction and are orientated downslope. They are interpreted as debris flow deposits. The widespread occurrence of debris flow deposits on the slope in this region supports the interpretation of an advance of the Greenland Ice Sheet to the shelf edge. The ice sheet delivered glacial sediment directly to the upper continental slope and this sediment was subsequently remobilised downslope by debris flow processes. Prominent submarine channels are present on swath bathymetric and TOPAS records from the lower continental slope in >2500 m water depth between 73° and 76° N. The channels incise acoustically stratified sediments that are likely the result of turbidity current deposition.
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SHIPBOARD ADCP Gwyn Griffiths (SOC) The RD Instruments 150 kHz shipboard ADCP (VM-150) was used throughout the cruise for current profile measurements. No technical problems were encountered. Key configuration parameters were: Ensemble interval: 2 minutes initially, then 5 minutes Cell length: 8 metres Number of cells: 50 Bottom tacking: enabled The instrument was set to use the computed sound velocity for correcting its velocity data. The usual clock drift within the PC was noted each day for later correction. Data processing used the ‘pstar’ route, via the Level C ‘adcp’ data stream, through a series of unix scripts on jrua. Ancillary measurements from the ship’s gyrocompass, the Ashtech ADU GPS-based heading reference and GPS position were acquired, processed and merged with the ADCP data as described in sequence below: gyroexec0 reads in gyro data, performs checks and appends to a gyro data file for the cruise (106gyr01). ashexec0 reads in Ashtech ADU data and edits the data based on limits set on the quality parameters mrms and brms. ashexec1 merges the Ashtech and gyro data, to give the heading difference a-ghdg. This is an especially important correction in high latitudes where the gyrocompass error is magnified by the secant of latitude (errors at 80° being nearly three times those at 60°). In addition transient errors of several degrees due to damped Schuler oscillations caused by sharp changes of course needed to be corrected. ashexec2 despikes the a-ghdg data and forms an average over 5 minutes. navexec0 reads in the ‘bestnav’ navigation data and calculates ship speed and distance run over the ground from successive fixes. navexec1 despikes the data and averages to 2 minutes. adpexec0 reads in the adcp data, splits the (ungridded) bottom track data from the gridded water column profiles. adpexec1 corrects the timing based on manual records of clock drift
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adpexec2 merges in the heading correction from the ashexec2 file adpexec3 applies the calibration to the velocity data adpexec4 merges in the smoothed navigation data and calculates absolute currents. These files (styled 106adp’jday’d.abs) are then appended to form cruise files, which are then averaged to 10 minutes. From these files velocity profiles or single depth maps can be produced. ASCII copies of these averaged concatenated data files were also made available for processing using Matlab ®. Calibration The initial calibration of the VM-150 was checked against GPS during two runs, each of over two hours, on the NW Icelandic shelf. The scale factor (A) was found to be 1.021 +/0.001 and the offset angle (phi) was –1.65°. That is, the ADCP vector needed to be rotated anticlockwise by 1.65 degrees. This calibration was at an indicated temperature of 15.8°C. Later, it became clear that this calibration was in error when operating in water temperatures of less than 0°. At these times, the ADCP transducer temperature was in the region of 6°C, but it is not immediately obvious that this is not the correct temperature within the transducer well. Nevertheless, a calibration on the Greenland shelf showed that while the offset angle was no different, the scaling factor should be 1.0426. ADCP data for day 230 onwards was recalibrated. This calibration was used until the end of day 240. Range and acoustic backscatter The range performance of the instrument was impressive. During this cruise, with calm conditions, in excess of 400 m range was usual. With the ship locked into an ice edge, the indicated currents were reasonable, although bottom track was lost and the backscatter profile was anomalous in showing a faster decay than would be expected from spherical spreading. An approximate calibration was applied to the acoustic backscatter from the VM-150 in order to assess the likely profiling range of the ADCPs on Autosub and for future reference against which the performance of Autosub’s ADCPs could be checked.
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Key ADCP and ancillary data files Instrument
Pstar master file
Version
ASCII master file
Notes
Gyrocompass
106gyr01
AS
106gyr01.asc
Covers day 226-242(1040)
Ashtech
106ash01.int
AO
106ash01.int.asc
Covers day 226-242(1040)
GPS
106gps01
AN
106gps01.asc
Covers day 226-242(1040)
GPS (bestnav)
abnv1061
DB
abnv1061.asc
Covers day 226-242(1040)
GPS (bestnav)
abnv1061.av
CD
abnv1061.av.asc
As above, 2 min average
ADCP (water)
106adp01.abs
BI
106adp01.abs.asc
Covers day 226-end 229
106adp01.abs.av
BE
106adp01.abs.av.asc
Iceland shelf calibration
106adp02.abs
AH
106adp02.abs.asc
106adp02.abs.av
AQ
106adp02.abs.av.asc
Covers day 230-end 240 Greenland shelf calibration
106adp03.abs
AA
106adp03.abs.asc
Covers day 241-242(1030)
106adp03.abs.av
AB
106adp03.abs.av.asc
Iceland shelf calibration
106bot01
AC
106bot01.asc
Covers day 226-end 229
ADCP (bottom)
Iceland shelf calibration 106bot02
AC
106bot02.asc
106bot03
AA
106bot03.asc
Covers day 230-end 240 Greenland shelf calibration Covers day 241-242(1030) Iceland shelf calibration
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LADCP Terry Edwards (UKORS), Guy Williams (ACECRC) and Pat Cooper (BAS) Introduction An upward s/n 1885 and downward s/n 4275 Lowered Acoustic Doppler Current Profiler (LADCP) was mounted on the CTD Rosette and deployed for each CTD cast during JCR106 to determine current velocity. Setup The downward looking LADCP was used as the master unit on all casts, reasons being purely historical. Master / slave synchronisation was carried out electronically between the two units. Casts 1 to 4 were set up using the script files in Part 1 of Appendix C. Casts 5 to 20 using the script files in Part 2 of Appendix C. The main differences being the number of pings per ensemble, time per ensemble, bin depths, number of bins and the ping interval. The RDI workhorse manual carries full descriptions of the parameter meanings and implications. Both upward and downward looking units have the “lowered” option enabled. This allows a degraded bottom track facility. Although bottom tracking accuracy is reduced, a separate bottom tracking ping is not required so that current velocity measurements are not degraded. Range of “lowered” bottom tracking is approximately 150m. Firmware version in both units was 16.18 Power was supplied to both units from a rechargeable battery pack mounted on the frame. Data downloaded using BBTALK software. Operation Cast 3 5 – 20
Problem Upward-looking instrument did not record / not initialised successfully Set-up file changed (Bin size, Bin No. Pings/Ensemble
Results A preliminary set of results were generated using MATLAB scripts from Martin Visbeck and Lamont-Doherty Earth Observatory, Version 7, 2002. All result files are provided on the JCR106 cruise data CD. Initial comparisons with the time-averaged Ship ADCP data for each cast were found to be promising (see below).
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Figure 1. LADCP (dashed) and Ship ADCP (thick) velocities (u – red, v – green) for Stn 6. The Ship ADCP data are the time average velocities over the duration of the LADCP/CTD cast.
Discussion The preliminary results show that the LADCP is fairly consistent in structure and magnitude with the ship- mounted ADCP for the majority of casts. Due to the lack of specialised expertise in processing the LADCP data on board JCR106, further work is expected to increase the accuracy of the results. This includes utilising the CTD data, ships navigation data and examining the bottom tracking capabilities of the instrument.
NERC Grant NER/T/S/2000/00985
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CONTINUOUS PLANKTON RECORDER Peter Wadhams A Hardy-Longhurst continuous plankton recorder (CPR) was deployed during the northward and southward passages of James Clark Ross. The recorder was provided by the Sir Alister Hardy Foundation for Ocean Science (SAHFOS), Plymouth. It consists of a towfish which funnels water through a collecting slit in which a section of silk is exposed, which is then wound against a second spool of silk and deposited in a formalin preservative bath. The recorder thus acts as a “tape recorder” for plankton types and quantities along track. Such recorders are towed behind merchant ships and provide a valuable survey of plankton variability in the ocean, but have not yet been used further north than Iceland. The instrument was invented by Sir Alister Hardy and was first used on the first of the Discovery Committee investigations in the Southern Ocean in 1924, as described in his book “Great Waters”. The recorder was deployed two hours out of Reykjavik and used as far as 77°N. On the return it was deployed at 77°36’N for the run back to Iceland. The cassette is changed every 500 n.ml., and four were used during the experiment.
NERC Grant NER/T/S/2000/00985
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ITS REPORT Doug Willis (BAS) 1. Netware / PCs There were no problems with JRNA during the cruise. 1.1. Workstations/Laptops A number of laptops were connected to the network of science use during the cruise. Most were Windows machines and connected using samba and the email was accessed using either IMAP or POP3. 2. AMOS Server No issues outstanding and the system worked well. 2.1. SUS and Sophos services Commissioned the Sophos and SUS services on JCR-AMOS-S1. The systems updated from BAS HQ and once they were up to date all the BAS supported machines were configured to collect their updates from these services. Two issues were found with configuring the workstations for the SUS service. •
Windows 2000 machines must be at service pack 3 before the update services work.
•
Some machines had hat the auto update service disabled in the services control panel thus preventing the updates from being collected from the server.
3. Data Logging Systems 3.1. Logging Currently logging the following sensors. Number
Sensor Name
Levc credat names
001
Glonass
gps_glos
015
GPS-ADU
gps_ash
023
Trimble
gps_nmea
029
Anemometer
anemom
032
TSSHRP
tsshrp
038
Oceanlogger
oceanlog
058
Emlog
em_log
060
Dopplerlog
dop_log
063
Simrad-ea500
sim500
065
Simrad-em120
em120
082
Winch
winch
096
Truewind-spd
097
Truewind-dir
098
Seatex
seatex
101
SeaSpy
seaspy
NERC Grant NER/T/S/2000/00985
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JR106 Cruise Report (v1.00)
NGYRO
ngyro
3.2. SCS The SCS data logging system performed well and there were no faults. Date
Time
Events
12/08/2004
08:19
Started logging
13/08/2004
15:51
AUD5 reset due to loss of heading information
26/08/2004
23:16
AUD5 reset due to loss of heading information
29/08/2004
18:00
Data logging stopped.
3.3. SCS data outputs. Two serial navigation streams were setup for this cruise. One containing the gyro heading was passed down to the main lab for the AutoSub team to use and one containing GPS navigation data was passed to the CTD deck unit in the UIC. 3.4. EM120 Swath / TOPAS The EM120 and Topas were run for most of the cruise. The EM120 became unstable once we reached latitudes of 78° or more. The first symptoms were that the helmsman display would crash when the maximize button was clicked. To avoid the crash first zoom in than expand. Later the helmsman display would not start at all. This fault was traced to the projection that was being used at the time. The setting was UTM. Changing this fixed the problems. The EM120 logging ma chine once ran out of disk space and had to have files removed from it to resolve this issue. The cause of this was the automated data checking routines were not functional on the Neptune system. This also caused a similar problem on the Topas machine. This has been resolved. During the course of the cruise the Neptune processing machine experienced three unexplained re-starts. The system is being monitored and the latest crash dump is to be analyzed to identify the fault. 4. Unix Systems 4.1. License managers. Currently the Uniras license manager is being run on JRUI as it will not run on Solaris 9 machines. There is an updated version at BAS that will be installed once the CODIS link is available to transfer the data. 5. Network Work began on the CODIS link. The dish was commissioned and a link established to BAS HQ. The router configuration needs some modifications and this is has been passed to Richard Cable. The 3com switches in the main lab were removed from their rack to try and trace the current fault. As yet no solution to their continued unreliability has presented its self. Work will continue on the next leg of the cruise.
NERC Grant NER/T/S/2000/00985
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JR106 Cruise Report (v1.00)
APPENDIX A - ICE STATION DATA Ice station 1, 20 August Went on ice 1510. Position 79º29.94’N, 14º24.54’W. Started Line 1 of holes parallel to ship’s head. 5 m intervals. Measured snow depth, freeboard, total ice thickness. Table 1: Line 1 Hole Snow cm position m 0 5 5 15,13,12 10 15,11,11 15 12,12,15 20 10,10,10 25 8,8,9 30 10,15,9 35 10,11,8 40 8,8,8 44-47 50 13,10,15 55 10,9,13 60 11,10,10 65 21,10,15 70 8.7.11 75 10,8,11 80 8,8,8 85 5,7,7 90 5,7,8 95 10,10,9 100 11,8,15
Freeboard cm
Thickness cm
Latitude
Longitude
Comments
9 13 12 15 12 12 13 16 15
145 147 160 175 170 175 173 195 162
79.4988861
-14.4091597
79.4988327
-14.4105759
23 20 18 27 20 25 31 28 12 2 28
167 170 222 220 226 193 250 196 193 161 198
79.4988174
-14.4114819
79.4987793
-14.4128284
79.498764
-14.4141111
Melt pool
Station 1: Line 1 100
0
-100
Thickness cm
-200
-300
-400
-500
-600
-700 0
50
100
150
200
Distance m Draft
NERC Grant NER/T/S/2000/00985
Freeboard
Snow
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Table 2: Line 2, parallel to Line 1, 5 m away, also from 0 to 100 pointing along line of ship. Hole position Snow cm Freeboard Thickness cm Latitude Longitude m cm 0 20,22,20 0 169 5 7,6,20 18 190 10 7,8,8 10 181 15 10,8,9 8 177 20 6,6,6 3 182 25 5,7,5 5 174 30 7,12,8 14 199 35 10,10,11 18 210 40 9,8,8 5 182 45 6,6,5 7 193 47-48 50 8,6,7 9 158 55 6,7,7 11 165 60 8,8,8 10 171 65 10,11,13 10 173 70 8,10,8 18 199 75 8,7,7 13 212 80 16,14,16 14 191 85 6,6,8 15 208 90 23,22,15 5 172 95 23,23,23 5 158 100 17,22,17 30 184
Commenst
Melt pool
Slushy
Station 1: Line 2 100
50
0
Thickness cm
-50
-100
-150
-200
-250
-300 0
20
40
60
80
100
Distance m Draft
Freeboard
Snow
Also took core at about centre of line 2. Two 1 m sections saved in deep freeze.
NERC Grant NER/T/S/2000/00985
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JR106 Cruise Report (v1.00)
Ice station 1 (cont.), 21 August Continued line 1 of holes parallel to ship’s head. 5 m intervals. Measured snow depth, freeboard, total ice thickness. Table 3: Line 1 (continued) Hole position Snow cm m 106.5 5,5,7
110 115 120 125 130 135 140 145 150 155 160 165 170 175 180 185 190 195 200
3,5,5 26,17,20 30.20.26 25.22.26 24.25.23 22,27,26 26.25.25 30,23 32 25,27,21 23.22.22 18,19,18 6,6,6 19,9,10 26,24,24 29,32,34 24,24,24 23,21,23 19,21,22 10,10,11
Freeboard cm 15
Thickness cm
86 19 6 5 3 4 10 8 3 4 13 20 11 0 4 1 1 3 5
763 180 164 177 208 228 225 201 162 228 250 266 206 148 158 180 177 183 157
Latitude
Longitude
709
Comments Edge of melt pond which lies just past yesterday’s 100 m mark Ridge Edge of ridge
79.4987106
-14.4151726
79.4986725
-14.4162245
79.4986572
-14.4178762
79.4986496
-14.4188099
Cross-line 50 m along new line (i.e. 150 m from start point), going 50 m to right R and 50- m to left L, with zero at centre. Table 4: Line 3, cross-line at 150 m on Line 1 Hole position Snow cm Freeboard Thickness cm m cm 0 (50R) 10,8.5,10 3 135 5 10 15 20 25 30 35 40 45 50
11,9,6 10,8,5 18,15,16.5 14,17,10 19,22,16 11,7,9 6,5,6 10.15.5,13 8.5,6,5.5 18,17,18
13 23 15 12 8 15 9 12 15 3
172 236 155 147 160 210 205 176 180 162
55 (5L)
17,19.5,17
10
207
60 65 70
22,19,20 20,22,19 9,12,10.5
12 13 27
214 223 201
NERC Grant NER/T/S/2000/00985
Latitude
Longitude
Comments
79.4981842
-14.4168091
Starting at far right
79.4984283
-14.4165087
79.4986725
-14.4164448
Same as 150 above in Table 3 Moving left from centre
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Autosub under Arctic Sea Ice 75 80 85 90 95 100
13,15,17 17,25,32 10,7,11 21,20,21 22,25,20 19,17,12
JR106 Cruise Report (v1.00) 11 13 16 13 18 16
185 177 176 176 177 175
79.4988937
-14.4163427
79.4991379
-14.4161329
Station 1: Line 3 100
50
0
Thickness cm
-50
-100
-150
-200
-250
-300 0
10
20
30
40
50
60
70
80
90
100
Distance m Draft
Freeboard
Snow
Cores – done near beginning of line. Core 1:
black tape is top 2 sections Top section is shorter than bottom
Core 2:
top section came in 5 pieces 2 sections Bottom section has short top bit, then long complete m core
NERC Grant NER/T/S/2000/00985
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JR106 Cruise Report (v1.00)
Ice station 2, 23 August Main line is along ship axis starting at stern. Cross line is R and L relative to looking forward. Cross lines run from 0 at centre to 50 at edges. The GPS measurements show that although the floe was once fast ice it has now become detached and is drifting at 0.138 knots south-east. Table 5: Line 1 (Main Line) Hole position Snow cm m 0 5,4,4 5 9,8,9 10 10,9,12 15 15,14,11 20 11,10,10 25 6,7,7 30 8,10,9 35 6,6,8 40 10,8,7
Freeboard cm 13 17 10 1 12 6 0 5 -0.5
Thickness cm
Latitude
Longitude
175 153 129 131 154 132 135 128 124
80.26732 80.26728 80.26726 80.26722 80.26719 80.26717 80.26711 80.26708 80.26707
-13.10927 -13.10963 -13.11013 -13.11046 -13.11075 -13.11109 -13.11154 -13.11196 -13.11233
45 50 55 60 65 70 75 80
9,9,9 9,11,10 6,5,6 5,4,6 6,6,7 6,8,5 7,10,8 15,15,16
6 9 10 10 9 14 8 -7
152 140 142 146 167 166 137 94
80.26704 80.26703 80.26701 80.26697 80.26693 80.26691 80.26690 80.26688
-13.11260 -13.11292 -13.11322 -13.11360 -13.11403 -13.11432 -13.11458 -13.11473
85 90 95 100
6,7,5 7,7,8 6,6,7 9,8,7
3 10 6 11
126 146 137 133
80.26683 80.26679 80.26676 80.26670
-13.11519 -13.11550 -13.11575 -13.11619
Comments
Flooded melt pool
Flooded melt pool
Station 2: Line 1 100
50
0
Thickness cm
-50
-100
-150
-200
-250
-300 0
10
20
30
40
50
60
70
80
90
100
Distance m Draft
NERC Grant NER/T/S/2000/00985
Freeboard
Snow
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JR106 Cruise Report (v1.00)
Table 6: Line 2, cross-line at 50 m on Line 1 Hole position Snow cm Freeboard m cm 50R 6,6,6 1 45R 12,12,12 20 40R 8,6,6 27 35R 7,6,6 6 30R 10,7,12 9 25R 7,7,7 10 20R 6,6,6 8 15R 7,7,7 13 10R 9,8,7 10 5R 7,6,6 11 0 9,11,10 9
5L 10L 15L 20L 25L 30L 35L 40L 45L 50L
6,6,6 6,6,6 6,6,9 7,6,6 7,10,10 6,5,6 6,6,7 5,5,5 6,7,8 7,7,7
Thickness cm
Latitude
Longitude
108 155 130 113 150 142 146 142 173 174 140
80.26748 80.26744 80.26738 80.26733 80.26731 80.26726 80.26722 80.26718 80.26716 80.26714 80.26703
-13.11135 -13.11130 -13.11117 -13.11108 -13.11106 -13.11110 -13.11113 -13.11119 -13.11124 -13.11133 -13.11292
154 158 167 169 166 150 120 135 122 138
80.26706 80.26703 80.26701 80.26699 80.26694 80.26691 80.26688 80.26685 80.26682 80.26676
-13.10913 -13.10897 -13.10868 -13.10833 -13.10767 -13.10742 -13.10713 -13.10697 -13.10665 -13.10633
12 12 8 13 15 12 9 9 10 4
Comments
Same as 150 above in Table 5
Station 2: Line 2 100
50
0
Thickness cm
-50
-100
-150
-200
-250
-300 0
10
20
30
40
50
60
70
80
90
100
Distance m Draft
Freeboard
Snow
Table 7: Snow samples Bottle no. Line/Hole 596 10L 540 20L 239 30L 234 40L 578 50L
NERC Grant NER/T/S/2000/00985
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JR106 Cruise Report (v1.00)
Ice station 3, 26 August Line 1 - Main line is along ship axis starting at stern. 0 is beginning of line nearest ship. Table 8: Line 1 Hole position m 0 5 10 15 20 25 30
Snow cm
Thickness cm
Latitude
Longitude
4,5,5 5,5,5 5,5,5 4,4,4 4,4,5 4,5,5 5,5,5
Freeboard cm 9 5 7 8 2 6 5
141 137 132 147 137 126 141
79.3316345
-13.848052
35
4,4,4
6
116
40 45 50
4,4,5 4,5,4 4,5,4
4 5 4
104 107 95
55 60
10,11,10 12,12,11
5 5
125 112
65 70 75 80 85 90 95 100 105 110 115 120 125 130 135 140 145 150 155 160 165 170 175 180 185 190 195 200
? 10,12,12 11,11,13 11,11,9 9,9,10 11,11,10 14,14,16 11,11,11 12,12,13 14,11,11 11,12,11 15,11,15 11,12,11 11,12,12 11,11,11 12,15,12 11,11,11 10,10,10 10,11,10 11,10,12 11,11,13 10,12,12 11,12,11 12,13,11 10,10,10 10,11,10 11,11,10 11,11,10
3 6 5 4 10 10 7 1 6 2 3 5 4 5 0 5 11 6 1 13 12 16 12 4 3 10 2 5
99 110 108 109 115 102 110 93 106 100 125 120 123 127 123 126 132 120 120 142 144 166 140 140 147 144 121 135
NERC Grant NER/T/S/2000/00985
Comments
Melt pond alongside Melt pond alongside
79.3312149
-13.8494577
Melt pool . Large melt pool runs parallel to line from 60 to 100
79.3308487
-13.8502512
79.3305588
-13.8513241
79.3299942
-13.8526011
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JR106 Cruise Report (v1.00)
Line 2 - Parallel to line 1 and about 40 m to right, looking from ship. Exact distance will be given by GPS. Table 9: Line 2 Hole position m. 0 5 10 15 20 25 30 35 40 45 50 55 60 65 70 75 80 85 90 95 100 100 105 110 115 120 125 130 135 140 145 150 155 160 165 170 175 180 185 190 195 200
Snow cm 11,12,12 10,10,11 10,11,10 10,10,10 11,11,11 11,11,12 12,12,12 10,10,11 12,12,12 10,10,10 12,11,11 10,10,10 10,11,12 10,10,10 10,11,11 10,10,11 10,11,11 10,10,11 9,10,11 12,12,12 11,10,11 12,12,11 11,11,11 14,14,14 10,13,13 13,12,11 11,11,11 12,12,12 13,13,13 10,10,10 13,14,12 12,12,11 10,11,12 13,13,17 11,11,11 14,14,14 14,14,11 12,11,11 15,29,26 9,14,13 9,10,9 11,12,11
Freeboard cm 11 10 15 8 8 4 4 3 8 13 9 12 3 8 11 10 7 6 11 10 10 6 17 10 10 10 8 5 7 7 10 4 5 15 5 3 3 7 12 14 8 6
NERC Grant NER/T/S/2000/00985
Thickness cm
Latitude
Longitude
146 143 151 145 133 148 130 128 147 146 156 151 142 139 152 156 149 148 156 170 170 193 155 151 149 140 180 163 171 139 168 130 163 159 139 135 132 132 158 162 149 155
79.3318634
-13.8500261
79.3314743
-13.8511581
79.3309708
-13.8520918
79.330574
-13.8527994
79.3301239
-13.8538189
Comments
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JR106 Cruise Report (v1.00)
Station 3: Line 1 100
50
0
Thickness cm
-50
-100
-150
-200
-250
-300 0
50
100
150
200
150
200
Distance m Draft
Freeboard
Snow
Station 3: Line 2 100
50
0
Thickness cm
-50
-100
-150
-200
-250
-300 0
50
100 Distance m Draft
NERC Grant NER/T/S/2000/00985
Freeboard
Snow
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JR106 Cruise Report (v1.00)
Ridge - Parallel to lines 1 and 2 and some 100 m to left, looking from ship. Holes are numbered in reverse, from 0 furthest from ship to 50 closest. Table 10: Ridge Hole position m 0 5
7 9 11 13 15 17 19 21 23 25 30 35 40 45 50
Line Snow cm
Thickness cm
Latitude
Longitude
11,10,11 11,11,11
Freeboard cm 4 -3
114 85
79.3316422
-13.8448706
9,11,9 11,11,11 12,12,12 9,9,10 10,11,10 9,10,9 10,14,14 10,10,10 9,9,10 11,10,10 13,10,20 10,10,10 10,10,9 12,12,11 12,12,13
-2 -2 6 47 90 70 8 5 8 8 7 12 11 12 17
89 100 120 245 297 190 112 106 107 112 126 126 120 120 143
Comments
Standing water on top of ice
79.3313217
-13.8455687
79.3311996
-13.8456812
Station 3: Line 3 - Ridge 100
50
0
Thickness cm
-50
-100
-150
-200
-250
-300 0
10
20
30
40
50
Distance m Draft
NERC Grant NER/T/S/2000/00985
Freeboard
Snow
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JR106 Cruise Report (v1.00)
APPENDIX B – SALINITIES SHIP------------- JCR CRUISE-------- JR106 leg 1 DATE----------Aug-04
SEABIRD C.T.D. SALINITY DATA CAST NO BOTTLE SAMPLE 1 1 crate4 1 1 2 2 1 13 3 1 14 4 2 1 5 2 2 6 2 3 7 2 4 8 4 1 9
4 5 5 5 5 6 6 6 6 7 7 7 7 9 9 9 9 10 10 10 10 11 11 11 11 12 12 12 12 13 13 13 13 14 14 14 14 15 15 15 15 17 17 17 17 18 18 18 18 19 19 19 19 20 20 20 20
13 1 2 3 4 1 2 3 4 1 2 3 4 3 4 13 14 1 2 13 13 1 2 13 14 1 2 13 14 1 2 13 14 1 2 3 4 1 2 3 4 1 2 13 14 1 2 13 14 1 2 13 14 1 2 13 14
11 13 14 15 16 17 18 19 20 21 22 23 24 crate 5 2 1 3 4 6 7 8 9 10 11 12 13 14 15 16 18 19 20 21 22 23 24 crate11 241 242 243 244 245 246 247 248 249 250 251 252 253 254 255 256 257 258 259 260 261 262
SAL PRI 34.9049 34.9051 34.9148 34.9148 34.7461 34.7468 34.5808 34.5799 34.5053
32.9128 32.8643 32.8642 32.8436 32.8427 33.3153 33.3309 32.8472 32.8473 33.5511 33.5525 32.8833 32.8828 32.9544 32.9645 32.8155 32.806 34.1528 34.2021 32.8845 32.8735 34.6125 34.6171 32.8316 32.8312 34.6465 34.6463 32.8482 32.8474 34.7249 34.7263 33.0475 32.9319 34.5802 34.5816 34.5362 34.5294 34.6361 34.6358 34.5084 34.5082 34.7295 34.7297 34.5219 34.5191 34.674 34.7067 34.5501 34.5502 34.7548 34.7549 33.0092 32.9997 34.9119 34.9119 34.9137 34.9138
SAL SEC SEC-PRI PORTASAL PRI-PORTASAL SEC-PORTASAL 34.904 -0.0009 34.9082 -0.0033 -0.0042 34.9043 -0.0008 34.9072 -0.0021 -0.0029 34.9143 -0.0005 34.9134 0.0014 0.0009 34.9137 -0.0011 34.9163 -0.0015 -0.0026 34.7455 -0.0006 34.7344 0.0117 0.0111 34.7454 -0.0014 34.738 0.0088 0.0074 34.5827 0.0019 34.6598 -0.079 -0.0771 34.5847 0.0048 34.6671 -0.0872 -0.0824 34.5044 -0.0009 34.4243 0.081 0.0801
32.9145 32.8643 32.864 32.8428 32.8425 33.3056 33.3246 32.8468 32.8469 33.5488 33.553 32.882 32.8819 32.9507 32.962 32.8135 32.8071 34.1363 34.1675 32.8968 32.8716 34.6115 34.6102 32.8304 32.8301 34.6438 34.6439 32.8474 32.846 34.7209 34.7251 33.0036 32.9627 34.5649 34.5778 34.5309 34.5276 34.6331 34.6343 34.5065 34.5049 34.7268 34.7265 34.5206 34.5185 34.6689 34.6969 34.5477 34.5469 34.7515 34.7516 33.0228 33.0157 34.9089 34.9089 34.9108 34.9108
0.0017 0 -0.0002 -0.0008 -0.0002 -0.0097 -0.0063 -0.0004 -0.0004 -0.0023 0.0005 -0.0013 -0.0009 -0.0037 -0.0025 -0.002 0.0011 -0.0165 -0.0346 0.0123 -0.0019 -0.001 -0.0069 -0.0012 -0.0011 -0.0027 -0.0024 -0.0008 -0.0014 -0.004 -0.0012 -0.0439 0.0308 -0.0153 -0.0038 -0.0053 -0.0018 -0.003 -0.0015 -0.0019 -0.0033 -0.0027 -0.0032 -0.0013 -0.0006 -0.0051 -0.0098 -0.0024 -0.0033 -0.0033 -0.0033 0.0136 0.016 -0.003 -0.003 -0.0029 -0.003
NERC Grant NER/T/S/2000/00985
32.9406 32.8847 32.8877 32.8632 32.8608 33.2862 33.3052 32.9019 32.9355 33.5432 33.5461 32.9124 32.9555 32.9305 32.9301 32.8349 32.8257 34.075 34.177 32.9291 32.8889 34.6071 34.6121 32.9551 32.8518 34.6367 34.6491 32.8844 32.8656 34.7076 34.7202 33.001 32.9661 34.5511 34.5641 34.5397 34.5452 34.631 34.6351 34.5206 34.5485 34.7246 34.7232 34.5548 34.5349 34.6832 34.692 34.5574 34.5547 34.75 34.752 33.2883 33.0825 34.9098 34.9089 34.9125 34.9116
-0.0278 -0.0204 -0.0235 -0.0196 -0.0181 0.0291 0.0257 -0.0547 -0.0882 0.0079 0.0064 -0.0291 -0.0727 0.0239 0.0344 -0.0194 -0.0197 0.0778 0.0251 -0.0446 -0.0154 0.0054 0.005 -0.1235 -0.0206 0.0098 -0.0028 -0.0362 -0.0182 0.0173 0.0061 0.0465 -0.0342 0.0291 0.0175 -0.0035 -0.0158 0.0051 0.0007 -0.0122 -0.0403 0.0049 0.0065 -0.0329 -0.0158 -0.0092 0.0147 -0.0073 -0.0045 0.0048 0.0029 -0.2791 -0.0828 0.0021 0.003 0.0012 0.0022
-0.0261 -0.0204 -0.0237 -0.0204 -0.0183 0.0194 0.0194 -0.0551 -0.0886 0.0056 0.0069 -0.0304 -0.0736 0.0202 0.0319 -0.0214 -0.0186 0.0613 -0.0095 -0.0323 -0.0173 0.0044 -0.0019 -0.1247 -0.0217 0.0071 -0.0052 -0.037 -0.0196 0.0133 0.0049 0.0026 -0.0034 0.0138 0.0137 -0.0088 -0.0176 0.0021 -0.0008 -0.0141 -0.0436 0.0022 0.0033 -0.0342 -0.0164 -0.0143 0.0049 -0.0097 -0.0078 0.0015 -0.0004 -0.2655 -0.0668 -0.0009 0 -0.0017 -0.0008
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APPENDIX C – LADCP SCRIPTS AND PROCESSING MESSAGES PART 1 Cast 1 to 4 script files enabling running parameters. SM1 indicates master, SM2 indicates slave. >CF11101 >EA00000 >EB00000 >ED00000 >ES35 >EX11111 >EZ0111111 >SM1 >SA001 >SI0 >SW75 >TE00:00:01.00 >TP00:01.00 >LD111100000 >LF0500 >LN016 >LP00003 >LS800 >LV250 >LJ1 >LW1 >LZ30,220 >CK [Parameters saved as USER defaults] >CS
>CF11101 >EA00000 >EB00000 >ED00000 >ES35 >EX11111 >EZ0111111 >SM2 >SA001 >ST0300 >TE00:00:01.00 >TP00:01.00 >LD111100000 >LF0500 >LN016 >LP00003 >LS800 >LV250 >LJ1 >LW1 >LZ30,220 >CK [Parameters saved as USER defaults] >CS
NERC Grant NER/T/S/2000/00985
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JR106 Cruise Report (v1.00)
PART 2 Cast 5 to 20 script files enabling running parameters. SM1 indicates master, SM2 indicates slave. >CF11101 >EA00000 >EB00000 >ED00000 >ES33 >EX11111 >EZ0111111 >SM1 >SA001 >SI0 >SW75 >TE00:00:02.72 >TP00:00.50 >LD111100000 >LF0500 >LN015 >LP00003 >LS1600 >LV250 >LJ1 >LW1 >LZ30,220 >CK [Parameters saved as USER defaults] >CS
>CF11101 >EA00000 >EB00000 >ED00000 >ES33 >EX11111 >EZ0111111 >SM2 >SA001 >ST0300 >TE00:00:02.72 >TP00:0.50 >LD111100000 >LF0500 >LN015 >LP00003 >LS1600 >LV250 >LJ1 >LW1 >LZ30,220 >CK [Parameters saved as USER defaults] >CS
NERC Grant NER/T/S/2000/00985
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JR106 Cruise Report (v1.00)
PART 3 – Preliminary Processing Error Messages Station1
WARNING WARNING
found 15 ensembles with bad checksum (d) found 15 ensembles with bad checksum (u)
warning mean ping rate not equal between both instruments up instrument is different by -91 ensembles found 13 bad bottom error velocities and discarded them removed 593 values because of high error velocity removed 4 bottom values because of high error velocity **
found
7
large horizontal velocities
no SADCP data will use 82 % of data --------------------------------------------------------------------Station2
WARNING found 15 ensembles with bad checksum WARNING found 15 ensembles with bad checksum warning mean ping rate not equal between both instruments up instrument is different by -88 ensembles found 23 bad bottom error velocities and discarded them removed 1591 values because of high error velocity removed 19 bottom values because of high error velocity removing 1039 values
below recognized bottom
can not find SADCP data file: will use 86 % of data --------------------------------------------------------------------Station3 Error – no upward (slave) file recorded
--------------------------------------------------------------------Station4
WARNING found 15 ensembles with bad checksum WARNING found 15 ensembles with bad checksum warning mean ping rate not equal between both instruments up instrument is different by -108 ensembles found 10 bad bottom error velocities and discarded them removed 1199 values because of high error velocity removed 7 bottom values because of high error velocity can not find SADCP data file: will use 75 % of data
-----------------Station5
script file changed (see appendix) ----------
WARNING found 15 ensembles with bad checksum WARNING found 15 ensembles with bad checksum best lag not obvious! use time to match up-down looking ADCP found 4 bad bottom error velocities and discarded them removed 1399 values because of high error velocity removed 23 bottom values because of high error velocity ** found 9 large horizontal velocities can not find SADCP data file: will use 83 % of data
NERC Grant NER/T/S/2000/00985
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JR106 Cruise Report (v1.00)
WARNING found 15 ensembles with bad checksum WARNING found 15 ensembles with bad checksum best lag not obvious! use time to match up-down looking ADCP found 6 bad bottom error velocities and discarded them removed 1302 values because of high error velocity removed 15 bottom values because of high error velocity
WARNING one bean might be weak ! weak up looking beam 2 Outlier discarded 199 bins down looking Outlier discarded 80 bins up looking no bottom found given maximum profile depth : 107 extracted bottom depth : 143 bottom depth error : 22 removing 944 values below recognized bottom can not find SADCP data file: no bottom track data will use 80 % of data --------------------------------------------------------------------Station 7
WARNING WARNING best lag mean lag
found 15 ensembles with bad checksum found 15 ensembles with bad checksum not obvious! use time to match up-down looking ADCP: is -108.9415 ensembles
found 3 bad bottom error velocities and discarded them removed 1429 values because of high error velocity removed 20 bottom values because of high error velocity **
found
11
large horizontal velocities
Outlier discarded 177 bins down looking Outlier discarded 86 bins up looking can not find SADCP data file: will use 85 % of data
Station 8
WARNING WARNING
found 15 ensembles with bad checksum found 15 ensembles with bad checksum
best lag not obvious! use time to match up-down looking ADCP: mean lag is -116.3464 ensembles found 9 bad bottom error velocities and discarded them removed 1483 values because of high error velocity removed 11 bottom values because of high error velocity Outlier discarded 189 bins down looking Outlier discarded 77 bins up looking
NERC Grant NER/T/S/2000/00985
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JR106 Cruise Report (v1.00)
WARNING one bean might be weak ! weak up looking beam 2 no SADCP data will use 78 % of data
Station 9
WARNING WARNING
found 15 ensembles with bad checksum found 15 ensembles with bad checksum
best lag not obvious! use time to match up-down looking ADCP mean lag is -129.7861 ensembles found 13 bad bottom error velocities and discarded them removed 887 values because of high error velocity removed 19 bottom values because of high error velocity Outlier discarded 158 bins down looking Outlier discarded 41 bins up looking no bottom found given maximum profile depth : 89 extracted bottom depth : 136 bottom depth error : 20 removing 1687 values below recognized bottom can not find SADCP data file: no bottom track data will use 80 % of data
Station 10
WARNING WARNING
found 15 ensembles with bad checksum found 15 ensembles with bad checksum
best lag not obvious! use time to match up-down looking ADCP mean lag is -129.0418 ensembles found 5 bad bottom error velocities and discarded them removed 925 values because of high error velocity removed 18 bottom values because of high error velocity Outlier discarded 204 bins down looking Outlier discarded 120 bins up looking can not find SADCP data file: will use 82 % of data
Station 11
WARNING WARNING
found 15 ensembles with bad checksum found 15 ensembles with bad checksum
best lag not obvious! use time to match up-down looking ADCP mean lag is -127.6158 ensembles WARNING one bean might be weak ! weak up looking beam 2 Outlier discarded 235 bins down looking
NERC Grant NER/T/S/2000/00985
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Outlier discarded 144 bins up looking no bottom found no SADCP data will use 80 % of data
Station 12
WARNING WARNING
found 15 ensembles with bad checksum found 15 ensembles with bad checksum
best lag not obvious! use time to match up-down looking ADCP mean lag is -130.5368 ensembles found 12 bad bottom error velocities and discarded them removed 852 values because of high error velocity removed 22 bottom values because of high error velocity **
found
7
large horizontal velocities
Outlier discarded 198 bins down looking Outlier discarded 141 bins up looking no bottom found removing 615 values below recognized bottom no SADCP data will use 82 % of data
Station 13
WARNING WARNING
found 15 ensembles with bad checksum found 15 ensembles with bad checksum
best lag not obvious! use time to match up-down looking ADCP mean lag is -124.4169 ensembles found 7 bad bottom error velocities and discarded them removed 429 values because of high error velocity removed 34 bottom values because of high error velocity Outlier discarded 290 bins down looking Outlier discarded 141 bins up looking no bottom found can not find SADCP data file: will use 81 % of data
Station 14
WARNING WARNING
found 15 ensembles with bad checksum found 15 ensembles with bad checksum
best lag not obvious! use time to match up-down looking ADCP mean lag is -112.2189 ensembles found 8 bad bottom error velocities and discarded them removed 966 values because of high error velocity removed 29 bottom values because of high error velocity
NERC Grant NER/T/S/2000/00985
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WARNING one bean might be weak ! weak up looking beam 2 Outlier discarded 241 bins down looking Outlier discarded 156 bins up looking no bottom found no bottom track data no SADCP data will use 84 % of data
Station 15
WARNING WARNING
found 15 ensembles with bad checksum found 15 ensembles with bad checksum
best lag not obvious! use time to match up-down looking ADCP mean lag is -92.751 ensembles found 9 bad bottom error velocities and discarded them removed 704 values because of high error velocity removed 25 bottom values because of high error velocity
Outlier discarded 216 bins down looking Outlier discarded 126 bins up looking no bottom found no SADCP data will use 83 % of data
Station 16
WARNING WARNING
found 15 ensembles with bad checksum found 15 ensembles with bad checksum
best lag not obvious! use time to match up-down looking ADCP mean lag is -111.2592 ensembles found 11 bad bottom error velocities and discarded them removed 707 values because of high error velocity removed 22 bottom values because of high error velocity Outlier discarded 213 bins down looking Outlier discarded 113 bins up looking no bottom found can not find SADCP data file: will use 80 % of data
Station 17
WARNING WARNING
found 15 ensembles with bad checksum found 15 ensembles with bad checksum
best lag not obvious! use time to match up-down looking ADCP mean lag is -109.1544 ensembles
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JR106 Cruise Report (v1.00)
found 14 bad bottom error velocities and discarded them removed 1103 values because of high error velocity removed 34 bottom values because of high error velocity Outlier discarded 303 bins down looking Outlier discarded 169 bins up looking no bottom found can not find SADCP data file: will use 85 % of data
Station 18
WARNING WARNING
found 15 ensembles with bad checksum found 15 ensembles with bad checksum
best lag not obvious! use time to match up-down looking ADCP mean lag is -112.6407 ensembles found 11 bad bottom error velocities and discarded them removed 898 values because of high error velocity removed 15 bottom values because of high error velocity WARNING one bean might be weak ! weak up looking beam 2 Outlier discarded 251 bins down looking Outlier discarded 181 bins up looking no bottom found can not find SADCP data file: will use 82 % of data
Station 19
WARNING WARNING
found 15 ensembles with bad checksum found 15 ensembles with bad checksum
best lag not obvious! use time to match up-down looking ADCP mean lag is -112.4509 ensembles found 7 bad bottom error velocities and discarded them removed 1019 values because of high error velocity removed 18 bottom values because of high error velocity **
found
6
large horizontal velocities
Outlier discarded 255 bins down looking Outlier discarded 156 bins up looking no bottom found no SADCP data
Station 20
will use 76 % of data found 15 bad bottom error velocities and discarded them removed 1031 values because of high error velocity removed 51 bottom values because of high error velocity
NERC Grant NER/T/S/2000/00985
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Outlier discarded 1227 bins down looking Outlier discarded 862 bins up looking no bottom found no bottom track data no SADCP data will use 72 % of data increased error because of shear - inverse difference
NERC Grant NER/T/S/2000/00985
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